Skip to main content

Advertisement

Log in

Asteroseismology and interferometry

  • Review Article
  • Published:
The Astronomy and Astrophysics Review Aims and scope

Abstract

Asteroseismology provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Recent developments, including the first systematic studies of solar-like pulsators, have boosted the impact of this field of research within astrophysics and have led to a significant increase in the size of the research community. In the present paper we start by reviewing the basic observational and theoretical properties of classical and solar-like pulsators and present results from some of the most recent and outstanding studies of these stars. We centre our review on those classes of pulsators for which interferometric studies are expected to provide a significant input. We discuss current limitations to asteroseismic studies, including difficulties in mode identification and in the accurate determination of global parameters of pulsating stars, and, after a brief review of those aspects of interferometry that are most relevant in this context, anticipate how interferometric observations may contribute to overcome these limitations. Moreover, we present results of recent pilot studies of pulsating stars involving both asteroseismic and interferometric constraints and look into the future, summarizing ongoing efforts concerning the development of future instruments and satellite missions which are expected to have an impact in this field of research.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  • Adorf HM (1995) Interpolation of irregularly sampled data series—a survey. In: Shaw RA, Payne HE, Hayes JJE (eds) Astronomical Data Analysis Software and Systems IV, ASP Conference Series vol 77, p 460

  • Aerts C (1996). Mode identification of pulsating stars from line–profile variations with the moment method: a more accurate discriminant. Astron Astrophys 314: 115–122

    ADS  Google Scholar 

  • Aerts C and De Cat P (2003). β Cep stars from a spectroscopic point of view. Space Sci Rev 105: 453–492

    Article  ADS  Google Scholar 

  • Aerts C, De Pauw M and Waelkens C (1992). Mode identification of pulsating stars from line profile variations with the moment method. an example—The Beta Cephei star Delta Ceti. Astron Astrophys 266: 294–306

    ADS  Google Scholar 

  • Aerts C, De Cat P, Peeters E, Decin L, De Ridder J, Kolenberg K, Meeus G, Van Winckel H, Cuypers J and Waelkens C (1999). Selection of a sample of bright southern Slowly Pulsating B Stars for long-term photometric and spectroscopic monitoring. Astron Astrophys 343: 872–882

    ADS  Google Scholar 

  • Aerts C, Thoul A, Daszyńska J, Scuflaire R, Waelkens C, Dupret MA, Niemczura E and Noels A (2003). Asteroseismology of HD 129929: core overshooting and nonrigid rotation. Science 300: 1926–1928

    Article  ADS  Google Scholar 

  • Aerts C, Cuypers J, De Cat P, Dupret MA, De Ridder J, Eyer L, Scuflaire R and Waelkens C (2004). Long-term multicolour photometry and high-resolution spectroscopy of the two γ Doradus stars HD 12901 and HD 48501. Astron Astrophys 415: 1079–1088

    Article  ADS  Google Scholar 

  • Aerts C, Marchenko SV, Matthews JM, Kuschnig R, Guenther DB, Moffat AFJ, Rucinski SM, Sasselov D, Walker GAH and Weiss WW (2006a). δ Ceti is not monoperiodic: seismic modeling of a β Cephei star from MOST space-based photometry. Astrophys J 642: 470–477

    Article  ADS  Google Scholar 

  • Aerts C, De Cat P, Kuschnig R, Matthews JM, Guenther DB, Moffat AFJ, Rucinski SM, Sasselov D, Walker GAH and Weiss WW (2006b). Discovery of the new slowly pulsating B star HD 163830 (B5 II/III) from MOST space-based photometry. Astrophys J 642: L165–L168

    Article  ADS  Google Scholar 

  • Aime C, Martin F, Petrov R, Ricort G and Kadiri S (1984). Measurement of submilliarcsecond speckle displacements using a cross spectrum analysis technique—test on atmospheric dispersion. Astron Astrophys 134: 354–359

    ADS  Google Scholar 

  • Aizenman M, Smeyers P and Weigert A (1977). Avoided crossing of modes of non-radial stellar oscillations. Astron Astrophys 58: 41–46

    ADS  Google Scholar 

  • Andersen J (1991). Accurate masses and radii of normal stars. Astron Astrophys Rev 3: 91–126

    Article  ADS  Google Scholar 

  • Antia HM and Basu S (2005). The discrepancy between solar abundances and helioseismology. Astrophys J 620: L129–L132

    Article  ADS  Google Scholar 

  • Antoci V, Breger M, Rodler F, Bischof K and Garrido R (2007). Is 44 Tauri an exceptional case among the δ Scuti stars?. Astron Astrophys 463: 225–232

    Article  ADS  Google Scholar 

  • Appourchaux T, Berthomieu G, Michel E, Ballot J, Barban C, Baudin F, Boumier P, De Ridder J, Floquet M, García RA, Garrido R, Goupil MJ, Lambert P, Lochard J, Mazumdar A, Neiner C, Poretti E, Provost J, Roxburgh I, Samadi R and Toutain T (2006). Evaluation of the scientific performances for the seismology programme. In: Friedlund, M, Baglin, A, Lochard, J, and Conroy, L (eds) The CoRoT mission pre-launch status. stellar seismology and planet finding, pp 429–441. ESA SP-1306, ESA Publications, Noordwijk

    Google Scholar 

  • Armstrong JT, Hummel CA, Quirrenbach A, Buscher DF, Mozurkewich D, Vivekanand M, Simon RS, Denison CS, Johnston KJ, Pan XP, Shao M and Colavita MM (1992a). The orbit of φ Cygni measured with long-baseline optical interferometry: component masses and absolute magnitudes. Astron J 104: 2217–2223

    Article  ADS  Google Scholar 

  • Armstrong JT, Mozurkewich D, Vivekanand M, Simon RS, Denison CS, johnston KJ, Pan XP, Shao M and Colavita MM (1992b). The orbit of Alpha Equulei measured with long-baseline optical interferometry -Component masses, spectral types, and evolutionary state. Astron J 104: 241–252

    Article  ADS  Google Scholar 

  • Armstrong JT, Mozurkewich D, Rickard LJ, Hutter DJ, Benson JA, Bowers PF, Elias NM II, Hummel CA, Johnston KJ, Buscher DF, Clark JH III, Ha L, Ling LC, White NM and Simon RS (1998). The navy prototype optical interferometer. Astrophys J 496: 550–571

    Article  ADS  Google Scholar 

  • Armstrong JT, Nordgren TE, Germain ME, Hajian AR, Hindsley RB, Hummel CA, Mozurkewich D and Thessin RN (2001). Diameters of δ Cephei and η Aquilae measured with the navy prototype optical interferometer. Astron J 121: 476–481

    Article  ADS  Google Scholar 

  • Armstrong JT, Mozurkewich D, Hajian AR, Johnston KJ, Thessin RN, Peterson DM, Hummel CA and Gilbreath GC (2006). The Hyades binary θ2 Tauri: Confronting evolutionary models with optical interferometry. Astron J 131: 2643–2651

    Article  ADS  Google Scholar 

  • Arnold L, Lagrange A, Mourard D, Riaud P, Ferrari M, Gillet S, Kern P, Koechlin L, Labeyrie A, Lardière O, Malbet F, Perrin G, Rousset G, Tallon M (2002) High angular resolution in 2010–2020: a comparison between possible post-VLT/VLTI instruments. In: Traub WA (ed) Interferometry for optical astronomy II., Proc. SPIE vol. 4838, pp 134–143

  • Asplund M (2005). New light on stellar abundance analysis: departures from LTE and homogeneity. Annu Rev Astron Astrophys 43: 481–540

    Article  ADS  Google Scholar 

  • Asplund M, Nordlund Å, Trampedach R, Allende Prieto C and Stein RF (2000). Line formation in solar granulation. I. Fe line shapes, shifts and asymmetries. Astron Astrophys 359: 729–742

    ADS  Google Scholar 

  • Asplund M, Grevesse N, Sauval AJ, Allende Prieto C and Blomme R (2005). Line formation in solar granulation. VI. C I, C I, CH and C2 lines and the photospheric C abundance. Astron Astrophys 431: 693–705

    Article  ADS  Google Scholar 

  • Aufdenberg JP, Ludwig HG and Kervella P (2005). On the limb darkening, spectral energy distribution, and temperature structure of Procyon. Astrophys J 633: 424–439

    Article  ADS  Google Scholar 

  • Aufdenberg JP, Mérand A, Coudédu Foresto V, Absil O, Di Folco E, Kervella P, Ridgway ST, Berger DH, Brummelaar TA ten, McAlister HA, Sturmann J, Sturmann L and Turner NH (2006). First results from the CHARA Array. VII. Long-baseline interferometric measurements of Vega consistent with a pole-on, rapidly rotating star. Astrophys J 645: 664–675

    Article  ADS  Google Scholar 

  • Aufdenberg JP, Ireland MJ, Mérand A, CoudéDu Foresto V, Absil O, Folco E Di, Kervella P, Bagnuolo WG, Gies DR, Ridgway ST, Berger DH, Ten Brummelaar TA, McAlister HA, Sturmann J, Sturmann L, Turner NH and Jacob AP (2007). Interferometric constraints on gravity darkening with application to the modeling of spica A & B. In: Hartkopf, WI, Guinan, EF, and Harmanec, P (eds) Binary stars as critical tools & tests in contemporary astrophysics, IAUS 240, pp 271–280. Cambridge University Press, UK

    Google Scholar 

  • Ausseloos M (2005) Seismic Studies of selected Beta Cephei stars: Beta Centauri, Nu Eridani and 12 Lacertae. PhD Thesis, Katholieke Universiteit Leuven, Belgium

  • Ausseloos M, Scuflaire R, Thoul A and Aerts C (2004). Asteroseismology of the β Cephei star ν Eridani: massive exploration of standard and non-standard stellar models to fit the oscillation data. Mon Not R Astr Soc 355: 352–358

    Article  ADS  Google Scholar 

  • Ausseloos M, Aerts C, Lefever K, Davis J and Harmanec P (2006). High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the β Cephei star β Centauri. Astron Astrophys 455: 259–269

    Google Scholar 

  • Backus G and Gilbert F (1968). The resolving power of gross Earth data. Geophys J R Astr Soc 16: 169–205

    MATH  ADS  Google Scholar 

  • Backus G and Gilbert F (1970). Uniqueness in the inversion of inaccurate gross Earth data. Phil Trans R Soc London, Ser A 266: 123–192

    Article  ADS  MathSciNet  Google Scholar 

  • Baglin A (2003). COROT: A minisat for pionnier science, asteroseismology and planets finding. Adv Space Res 31(2): 345–349

    Article  ADS  Google Scholar 

  • Bagnuolo WG Jr and Hartkopf WI (1989). Binary star orbits from speckle interferometry. III - The evolution of the Capella stars. Astron J 98: 2275–2279

    Article  ADS  Google Scholar 

  • Bagnuolo WG, Taylor SF, McAlister HA, ten Brummelaar T, Gies DR, Ridgway ST, Sturmann J, Sturmann L, Turner NH, Berger DH and Gudehus D (2006). First results from the CHARA Array. V. Binary star astrometry: the case of 12 Persei. Astrophys J 131: 2695–2699

    ADS  Google Scholar 

  • Bahcall JN, Serenelli AM and Basu S (2006). 10,000 standard solar models: a Monte Carlo simulation. Astrophys J Suppl 165: 400–431

    Article  ADS  Google Scholar 

  • Baker NH (1987). Time dependent convection in stars—a review of the theories. In: Hillebrandt, W, Meyer-Hofmeister, E and Thomas, HC (eds) Physical processes in comets, stars and active galaxies, pp 105–124. Springer, Berlin

    Google Scholar 

  • Baker NH and Gough DO (1979). Pulsations of model RR Lyrae stars. Astrophys J 234: 232–244

    Article  ADS  Google Scholar 

  • Baker N and Kippenhahn R (1962). The pulsations of models of δ Cephei stars. Z Astrophys 54: 115–151

    ADS  Google Scholar 

  • Baker N and Kippenhahn R (1965). The pulsations of models of delta Cephei stars. II. Astrophys J 142: 868–889

    Article  ADS  Google Scholar 

  • Baldwin JE and Haniff CA (2002). The application of interferometry to optical astronomical imaging. Phil Trans A 360: 969–986

    Article  ADS  Google Scholar 

  • Baldwin JE, Beckett MG, Boysen RC, Burns D and Buscher DF (1996). The first images from an optical aperture synthesis array: mapping of Capella with COAST at two epochs. Astron Astrophys 306: L13–L16

    ADS  Google Scholar 

  • Ballot J, García RA and Lambert P (2006). Rotation speed and stellar axis inclination from modes: how CoRoT would see other suns. Mon Not R Astr Soc 369: 1281–1286

    Article  ADS  Google Scholar 

  • Balmforth NJ (1992). Solar pulsational stability. I: Pulsation-mode thermodynamics. Mon Not R Astr Soc 255: 603–631

    ADS  Google Scholar 

  • Balmforth NJ, Cunha MS, Dolez N, Gough DO and Vauclair S (2001). On the excitation mechanism in roAp stars. Mon Not R Astr Soc 323: 362–372

    Article  ADS  Google Scholar 

  • Balona LA (1986a). Mode identification from line profile variations. Mon Not R Astr Soc 219: 111–129

    ADS  Google Scholar 

  • Balona LA (1986b). Mode identification from line profile variations. II—A quantitative least-squares algorithm. Mon Not R Astr Soc 220: 647–656

    ADS  Google Scholar 

  • Balona LA (1987). Mode identification from line profile variations. III—Temperature variation and toroidal modes. Mon Not R astr Soc 224: 41–52

    ADS  Google Scholar 

  • Balona LA, Aerts C and Stefl S (1999). Simultaneous photometry and spectroscopy of the Be star 28 (omega) CMa—II. Line profile modelling. Mon Not R ast Soc 305: 519–526

    Article  ADS  Google Scholar 

  • Balona LA and Evers EA (1999). Mode identification and asteroseismology of δ Scuti stars. Mon Not R Astr Soc 302: 349–361

    Article  ADS  Google Scholar 

  • Balona LA and Stobie RS (1979). The effect of radial and non-radial stellar oscillations on the light, colour and velocity variations. Mon Not R Astr Soc 189: 649–658

    ADS  Google Scholar 

  • Bedding TR, Butler RP, Kjeldsen H, Baldry IK, O’Toole SJ, Tinney CG, Marcy GW, Kienzle F and Carrier F (2001). Evidence for solar-like oscillations in hydri. Astrophys J 549: L105–L108

    Article  ADS  Google Scholar 

  • Bedding TR, Kjeldsen H, Butler RP, McCarthy C, Marcy GW, O’Toole SJ, Tinney CG and Wright JT (2004). Oscillation frequencies and mode lifetimes in α Centauri A. Astrophys J 614: 380–385

    Article  ADS  Google Scholar 

  • Bedding TR, Butler RP, Carrier F, Bouchy F, Brewer BJ, Eggenberger P, Grundahl F, Kjeldsen H, McCarthy C, Nielsen TB, Retter A and Tinney CG (2006). Solar-like oscillations in the metal-poor subgiant ν Indi: constraining the mass and age using asteroseismology. Astrophys J 647: 558–563

    Article  ADS  Google Scholar 

  • Bedding TR, Kjeldsen H, Arentoft T, Bouchy F, Brandbyge J, Brewer BJ, Butler P, Christensen-Dalsgaard J, Dall T, Frandsen S, Karoff C, Kiss LL, Monteiro MJPFG, Pijpers FP, Teixeira TC, Tinney CG, Baldry IK, Carrier F and O’Toole SJ (2007). Solar-like oscillations in the G2 subgiant beta Hydri from dual-site observations. Astrophys J 663: 1315–1324

    Article  ADS  Google Scholar 

  • Basri G, Borucki WJ and Koch D (2005). The Kepler Mission: A wide-field transit search for terrestrial planets. NewAR 49: 478–485

    Article  ADS  Google Scholar 

  • Basu S, Chaplin WJ, Christensen-Dalsgaard J, Elsworth Y, Isaak GR, New R, Schou J, Thompson MJ and Tomczyk S (1997). Solar internal sound speed as inferred from combined BiSON and LOWL oscillation frequencies. Mon Not R Astr Soc 292: 243–251

    ADS  Google Scholar 

  • Basu S, Christensen-Dalsgaard J and Thompson MJ (2002). SOLA inversions for the core structure of solar-type stars. In: Favata, F, Roxburgh, IW, and Galadí-Enríquez, D (eds) Proc. 1st Eddington workshop, ‘stellar structure and habitable planet finding’, ESA SP-, pp 249–252. ESA Publications Division, Noordwijk

    Google Scholar 

  • Basu S., Mazumdar A, Antia HM and Demarque P (2004). Asteroseismic determination of helium abundance in stellar envelopes. Mon Not R Astr Soc 350: 277–286

    Article  ADS  Google Scholar 

  • Basu S, Chaplin WJ, Elsworth Y, New R, Serenelli AM and Verner GA (2007). Solar abundances and helioseismology: fine-structure spacings and separation ratios of low-degree p-modes. Astrophys J 655: 660–671

    Article  ADS  Google Scholar 

  • Batchelor GK (1953). The theory of homogeneous turbulence. Cambridge University Press, UK

    MATH  Google Scholar 

  • Beckers JM (1982). Differential speckle interferometry. J Modern Optics 29: 361–362

    Article  ADS  MathSciNet  Google Scholar 

  • Bedding TR, Kjeldsen H (2006) Observations of solar-like oscillations. In: Fletcher K, Thompson M (eds)Proc. of SOHO 18/GONG 2006/HELAS I, Beyond the spherical Sun, ESA SP-624, pp 1–5

  • Bedding TR, Kjeldsen H (2007) Asteroseismology from solar-like oscillations. In: Proc. of the 14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, ASP conference Series (in press)

  • Bennett PD, Harper GM, Brown A and Hummel CA (1996). The masses and radii of the eclipsing binary ζ Aurigae. Astrophys J 471: 454–479

    Article  ADS  Google Scholar 

  • Benson JA, Hutter DJ, Elias NM, Bowers PF, Johnston KJ, Hajian AR, Armstrong JT, Mozurkewich D, Pauls TA, Rickard LJ, Hummel CA, White NM, Black D and Denison CS (1997). Multichannel optical aperture synthesis imaging of ζ1 Ursae Maioris with the navy prototype optical interferometer. Astron J 114: 1221–1226

    Article  ADS  Google Scholar 

  • Berdyugina SV, Telting JH and Korhonen H (2003a). Surface imaging of stellar non-radial pulsations. I. Inversions of simulated data. Astron Astrophys 406: 273–280

    Article  ADS  Google Scholar 

  • Berdyugina SV, Telting JH, Korhonen H and Schrijvers C (2003b). Surface imaging of stellar non-radial pulsations. II. The β Cepheii star ω1 Sco. Astron Astrophys 406: 281–285

    Article  ADS  Google Scholar 

  • Berger DH, Gies DR, McAlister HA, ten Brummelaar TA, Henry TJ, Sturmann J, Sturmann L, Turner NH, Ridgway ST, Aufdenberg JP and Mérand A (2006). First results from the CHARA Array. IV. The interferometric radii of low-mass stars. Astrophys J 644: 475–483

    Article  ADS  Google Scholar 

  • Bergeron J, Monnet G (2002) Scientific drivers for ESO future VLT/VLTI instrumentation. ESO astrophysics symposia, Springer, Hidelberg, ISBN: 3-540-43755-X

  • Bevington PR and Robinson DK (2003). Data reduction and error analysis for the physical sciences, 3rd ed. McGraw-Hill, New York

    Google Scholar 

  • Bigot L and Dziembowski WA (2002). The oblique pulsator model revisited. Astron Astrophys 391: 235–245

    Article  ADS  Google Scholar 

  • Bigot L, Provost J, Berthomieu G, Dziembowski WA and Goode PR (2000). Non-axisymmetric oscillations of roAp stars. Astron Astrophys 356: 218–233

    ADS  Google Scholar 

  • Bigot L, Kervella P, Thévenin F and Ségransan D (2006). The limb darkening of α Centauri B. Matching 3(hydrodynamical models with interferometric measurements. Astron Astrophys 446): 635–641

    Google Scholar 

  • Blackwell DE and Shallis MJ (1977). Stellar angular diameters from infrared photometry. Application to Arcturus and other stars with effective temperatures. Mon Not Roy Astr Soc 180: 177–191

    Google Scholar 

  • Bloomfield P (1976). Fourier analysis of time series: an introduction. Wiley, New York

    MATH  Google Scholar 

  • Boden AF and Lane BF (2001). A preliminary visual orbit of BY Draconis. Astrophys J 547: 1071–1076

    Article  ADS  Google Scholar 

  • Boden AF, Koresko CD, van Belle GT, Colavita MM, Dumont PJ, Gubler J, Kulkarni SR, Lane BF, Mobley D, Shao M, Wallace JK, The PTI Collaboration and Henry GW (1999a). The visual orbit of ı Pegasi. Astrophys J 515: 356–364

    Article  ADS  Google Scholar 

  • Boden AF, Lane BF, Creech-Eakman MJ, Colavita MM, Dumont PJ, Gubler J, Koresko CD, Kuchner MJ, Kulkarni SR, Mobley DW, Pan XP, Shao M, van Belle GT, Wallace JK and Oppenheimer BR (1999b). The visual orbit of 64 Piscium. Astropys J 527: 360–368

    Article  ADS  Google Scholar 

  • Boden AF, Creech-Eakman MJ and Queloz D (2000). The visual orbit and evolutionary state of 12 Bootis. Astrophys J 536: 880–890

    Article  ADS  Google Scholar 

  • Boden AF, Sargent AI, Akeson RL, Carpenter JM, Torres G, Latham DW, Soderblom DR, Nelan E, Franz OG and Wasserman LH (2005a). Dynamical masses for low-mass pre-main-sequence stars: a preliminary physical orbit for HD 98800 B. Astrophys J 635: 442–451

    Article  ADS  Google Scholar 

  • Boden AF, Torres G and Hummel CA (2005b). Testing stellar models with an improved physical orbit for 12 bootis. Astrophys J 627: 464–476

    Article  ADS  Google Scholar 

  • Boden AF, Torres G and Latham DW (2006). A physical orbit for the high proper motion binary HD 9939. Astrophys J 644: 1193–1201

    Article  ADS  Google Scholar 

  • Boden AF, Torres G, Sargent AI, Akeson RL, Carpenter JM, Boboltz DA, Massi M, Ghez AM, Latham DW, Johnston KJ, Menten KM, Ros E (2007) Dynamical masses for pre-main sequence stars: a preliminary physical orbit for V773 Tau A. Astrophys J, astro-ph/02376 (in press)

  • Böhm-Vitense E (1958). Über die Wasserstoffkonvektionszone in Sternen verschiedener Effektivtemperaturen und Leuchtkräfte. Z Astrophys 46: 108–143

    ADS  Google Scholar 

  • Bordé P, Coudé du Foresto V, Chagnon G and Perrin G (2002). A catalogue of calibrator stars for long baseline stellar interferometry. Astron Astrophys 393: 183–193

    Article  ADS  Google Scholar 

  • Bouchy F and Carrier F (2002). The acoustic spectrum of α Cen A. Astron Astrophys 390: 205–212

    Article  ADS  Google Scholar 

  • Bradley PA and Winget DE (1994). An asteroseismological determination of the structure of the DBV white dwarf GD 358. Astrophys J 430: 850–857

    Article  ADS  Google Scholar 

  • Bradley PA, Winget DE and Wood MA (1993). The potential for asteroseismology of DB white dwarfs. Astrophys J 406: 661–673

    Article  ADS  Google Scholar 

  • Brassard P, Fontaine G (2004) Asteroseismology of the Crystallized ZZ Ceti Star BPM 37093: a Different View (part I). In: Danesy D (ed) SOHO 14 GONG 2004 workshop: helio- and asteroseismology: towards a golden future, ESA SP-559, pp 333–336

  • Brassard P, Fontaine G and Wesemael F (1995). The modeling of energy distributions and light curves of ZZ Ceti stars. 1: Basic theory and semianalytic expressions for the emergent flux. Astrophys J Suppl 96: 545–580

    Article  ADS  Google Scholar 

  • Breger M (2000). The multiperiodic δ Scuti star 4 Canum Venaticorum: amplitude variability. Mon Not R Astr Soc 313: 129–135

    Article  ADS  Google Scholar 

  • Breger M and Pamyatnykh AA (2006). Amplitude variability or close frequencies in pulsating stars—the δ Scuti star FG Vir. Mon Not R Astr Soc 368: 571–578

    Article  ADS  Google Scholar 

  • Breger M, Pamyatnykh AA, Zima W, Garrido R, Handler G and Reegen P (2002). Pulsation of the δ Scuti star θ2 Tau: new multisite photometry and modelling of instability. Mon Not R Astr Soc 336: 249–258

    Article  ADS  Google Scholar 

  • Breger M, Lenz P, Antoci V, Guggenberger E, Shobbrook RR, Handler G, Ngwato B, Rodler F, Rodriguez E, López de Coca P and Costa V (2005). Detection of 75 +  pulsation frequencies in the δ Scuti star FG Virginis. Astron Astrophys 435: 955–965

    Article  ADS  Google Scholar 

  • Briquet M and Aerts C (2003). A new version of the moment method, optimized for mode identification in multiperiodic stars. Astron Astrophys 398: 687–696

    Article  ADS  Google Scholar 

  • Brewer BJ, Bedding TR, Kjeldsen H and Stello D (2007). Baysian inference from observations of solar-like oscillations. Astrophys J 654: 551–557

    Article  ADS  Google Scholar 

  • Brickhill AJ (1983). The pulsations of ZZ Ceti stars. Mon Not R Astr Soc 204: 537–556

    ADS  Google Scholar 

  • Brickhill AJ (1991). The pulsations of ZZ Ceti stars—III. The driving mechanism. Mon Not R ast Soc 251: 673–680

    ADS  Google Scholar 

  • Brookes JR, Isaak GR and van der Raay HB (1978). The observation of a rotating body using high-resolution spectroscopy. Mon Not R Astr Soc 185: 19–22

    ADS  Google Scholar 

  • Brown TM, Gilliland RL, Noyes RW and Ramsey LW (1991). Detection of possible p-mode oscillations on Procyon. Astrophys J 368: 599–609

    Article  ADS  Google Scholar 

  • Brown TM, Christensen-Dalsgaard J, Mihalas B and Gilliland RL (1994). The effectiveness of oscillation frequencies in constraining stellar model parameters. Astrophys J 427: 1013–1034

    Article  ADS  Google Scholar 

  • Buscher DF, Bakker EJ, Coleman TA, Creech-Eakman MJ, Haniff CA, Jurgenson CA, Klinglesmith DA, Parameswariah CB, Young JS (2006) The Magdalena Ridge Observatory Interferometer: a high-sensitivity imaging array. In: Gamiz VL, Idell PS, Strojnik MS (eds) Unconventional imaging II, Proc. of the SPIE 6307, pp 63070B

  • Bruntt H, Kjeldsen H, Buzasi DL and Bedding TR (2005). Evidence for granulation and oscillations in Procyon from photometry with the WIRE satellite. Astrophys J 633: 440–446

    Article  ADS  Google Scholar 

  • Butler RP, Bedding TR, Kjeldsen H, McCarthy C, O’Toole SJ, Tinney CG, Marcy GW and Wright JT (2004). Ultra-high-precision velocity measurements of oscillations in α Centauri A. Astrophys J 600: L75–L78

    Article  ADS  Google Scholar 

  • Buzasi DL, Bruntt H, Bedding TR, Retter A, Kjeldsen H, Preston HL, Mandeville WJ, Suarez JC, Catanzarite J, Conrow T and Laher R (2005). Altair: The Brightest δ Scuti Star. Astrophys J 619: 1072–1076

    Article  ADS  Google Scholar 

  • Canuto VM and Mazzitelli I (1991). Stellar turbulent convection: a new model and applications. Astrophys J 370: 295–311

    Article  ADS  Google Scholar 

  • Canuto VM and Mazzitelli I (1992). Further improvements of a new model for turbulent convection in stars. Astrophys J 389: 724–730

    Article  ADS  Google Scholar 

  • Canuto VM, Goldman I and Mazzitelli I (1996). Stellar turbulent convection: a self-consistent model. Astrophys J 473: 550–559

    Article  ADS  Google Scholar 

  • Carpenter KG, Schrijver CJ, Karovska M (2005) SI—The Stellar imager: results from the vision mission study. In: American Astronomical Society Meeting 207, 07, Bulletin of the American Astronomical Society, vol 37, p. 1196

  • Carrier F. and Bourban G. (2003). Solar-like oscillations in the K1 dwarf star α Cen B. Astron Astrophys 406: L23–L26

    Article  ADS  Google Scholar 

  • Carrier F, Bouchy F, Kienzle F, Bedding TR, Kjeldsen H, Butler RP, Baldry IK, O’Toole SJ, Tinney CG and Marcy GW (2001). Solar-like oscillations in vec Hydri: Confirmation of a stellar origin for the excess power. Astron Astrophys 378: 142–145

    Article  ADS  Google Scholar 

  • Carrier F, Eggenberger P and Bouchy F (2005). New seismological results on the G0IV η Bootis. Astron Astrophys 434: 1085–1095

    Article  ADS  Google Scholar 

  • Carrier F, Kjeldsen H, Bedding TR, Brewer BJ, Butler RP, Eggenberger P, Grundahl F, McCarthy C, Retter A and Tinney CG (2007). Solar-like oscillations in the metal-poor subgiant ν Indi. II. Acoustic spectrum and mode lifetime. Astron Astrophys 470: 1059–1063

    Article  ADS  Google Scholar 

  • Castanheira BG, Nitta A, Kepler SO, Winget DE and Koester D (2005). HST observations of the pulsating white dwarf GD 358. Astron Astrophys 432: 175–179

    Article  ADS  Google Scholar 

  • Catala C, Aerts C, Aigrain S, Antonello E, Appourchaux T, Auvergne M, Baglin A, Barge P, Barstow MA, Baudin F, Boumier P, Cameron AC, Christensen-Dalsgaard J, Cutispoto G, Deeg H, Deleuil M, Desidera S, Donati JF, Favata F, Foing BH, Gameiro JF, Garcia R, Garrido F, Horne K, Lanza AF, Lanzafame AC, Lecavelierdes Etangs A, Lóger A, Mas-Hesse M, Messina S, Micela G, Michel E, Monteiro MJPFG, Mosser B, Noels A, Pagano I, Piotto G, Poretti E, Rauer H, Roca-Cortes T, Rodono M, Rouan D, Roxburgh I, Schneider J, Strassmeier K, Turck-Chièze S, Vauclair S, Vidal-Madjar A, Weiss WW and Wheatley P (2005). The Life of Stars and Their Planets. In: Favata, F, Sanz-Forcada, J, and Gimónez, A (eds) Proc. 39th ESLAB symposium on trends in space science and cosmic vision 2020, ESA SP-588, pp 99–104. Noordwijk, The Netherlands

    Google Scholar 

  • Chandrasekhar S (1964). A general variational principle governing the radial and the non-radial oscillations of gaseous masses. Astrophys J 139: 664–674

    Article  MATH  ADS  MathSciNet  Google Scholar 

  • Chaplin WJ, Elsworth Y, Isaak GR, Marchenkov KI, Miller BA, New R, Pinter B and Appourchaux T (2002a). Peak finding at low signal-to-noise: low-â„“ solar acoustic eigenmodes at n ≤ 9 from the analysis of BiSON data. Mon Not R Astr Soc 336: 979–991

    Article  ADS  Google Scholar 

  • Chaplin WJ, Elsworth Y, Isaak GR, Miller BA and New R (2002b). On the measurement precision of solar p-mode eigenfrequencies. Mon Not R Astr Soc 330: 731–736

    Article  ADS  Google Scholar 

  • Chaplin WJ, Houdek G, Elsworth Y, Gough DO, Isaak GR and New R (2005). On model predictions of the power spectral density of radial solar p modes. Mon Not R Astr Soc 360: 859–868

    Article  ADS  Google Scholar 

  • Chaplin WJ, Appourchaux T, Baudin F, Boumier P, Elsworth Y, Fletcher ST, Fossat E, García RA, Isaak GR, Jimónez A, Jimónez-Reyes SJ, Lazrek M, Leibacher JW, Lochard J, New R, Palló P, Rógulo C, Salabert D, Seghouani N, Toutain T and Wachter R (2006). Solar FLAG hare and hounds: on the extraction of rotational p-mode splittings from seismic, Sun-as-a-star data. Mon Not R Astr Soc 369: 985–996

    Article  ADS  Google Scholar 

  • Chaplin WJ, Elsworth Y, Miller BA and Verner GA (2007). Solar p-mode frequencies over three solar cycles. Astrophys J 659: 1749–1760

    Article  ADS  Google Scholar 

  • Chelli A and Petrov RG (1995). Model fitting and error analysis for differential interferometry. II. Application to rotating stars and binary systems. Astron Astophys Suppl Ser 109: 401–415

    ADS  Google Scholar 

  • Chlebowski T (1978). Nonradial oscillations of slowly rotating white dwarfs. Acta Astron 28: 441–463

    ADS  Google Scholar 

  • Christensen-Dalsgaard J (1980). On adiabatic non-radial oscillations with moderate or large l. Mon Not R Astr Soc 190: 765–791

    ADS  Google Scholar 

  • Christensen-Dalsgaard J (1982). On solar models and their periods of oscillation. Mon Not R Astr Soc 199: 735–761

    ADS  Google Scholar 

  • Christensen-Dalsgaard J (1984). What will asteroseismology teach us?. In: Mangeney, A and Praderie, F (eds) Space research prospects in stellar activity and variability, pp 11–45. Paris Observatory Press, Paris

    Google Scholar 

  • Christensen-Dalsgaard J (1988). A Hertzsprung-Russell diagram for stellar oscillations. In: Christensen-Dalsgaard, J and Frandsen, S (eds) Proc. IAU symposium No 123, advances in helio- and asteroseismology, pp 295–298. Reidel, Dordrecht

    Google Scholar 

  • Christensen-Dalsgaard J (1989). The effect of rotation on whole-disc Doppler observations of solar oscillations. Mon Not R Astr Soc 239: 977–994

    ADS  Google Scholar 

  • Christensen-Dalsgaard J (1991). Some aspects of the theory of solar oscillations. Geophys Astrophys Fluid Dyn 62: 123–152

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J (2002). Helioseismology. Rev Mod Phys 74: 1073–1129

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J (2004). Physics of solar-like oscillations. Solar Phys 220: 137–168

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J (2007) ASTEC – the Aarhus STellar evolution code. Astrophys Space Sci (in press)

  • Christensen-Dalsgaard J and Berthomieu G (1991). Theory of solar oscillations. In: Cox, AN, Livingston, WC and Matthews, M (eds) Solar interior and atmosphere, Space science series, pp 401–478. University of Arizona Press, Arizona

    Google Scholar 

  • Christensen-Dalsgaard J and Frandsen S (1983). Stellar 5 min oscillations. Solar Phys 82: 469–486

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J and Gough DO (1980). Is the Sun helium-deficient?. Nature 288: 544–547

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J and Gough DO (1982). On the interpretation of five-minute oscillations in solar spectrum line shifts. Mon Not R Astr Soc 198: 141–171

    ADS  Google Scholar 

  • Christensen-Dalsgaard J and Thompson MJ (1997). On solar p-mode frequency shifts caused by near-surface model changes. Mon Not R Astr Soc 284: 527–540

    ADS  Google Scholar 

  • Christensen-Dalsgaard J, Duvall TL Jr, Gough DO, Harvey JW and Rhodes EJ Jr (1980). Speed of sound in the solar interior. Nature 315: 378–382

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J, Gough DO and Libbrecht KG (1989). Seismology of solar oscillation line widths. Astrophys J 341: L103–L106

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J, Bedding TR and Kjeldsen H (1995). Modelling solar-like oscillations in η Bootis. Astrophys J 443: L29–L32

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J, Däppen W, Ajukov SV, Anderson ER, Antia HM, Basu S, Baturin VA, Berthomieu G, Chaboyer B, Chitre SM, Cox AN, Demarque P, Donatowicz J, Dziembowski WA, Gabriel M, Gough DO, Guenther DB, Guzik JA, Harvey JW, Hill F, Houdek G, Iglesias CA, Kosovichev AG, Leibacher JW, Morel P, Proffitt CR, Provost J, Reiter J, Rhodes EJ Jr, Rogers FJ, Roxburgh IW, Thompson MJ and Ulrich RK (1996). The current state of solar modeling. Science 272: 1286–1292

    Article  ADS  Google Scholar 

  • Christensen-Dalsgaard J, Arentoft T, Brown TM, Gilliland RL, Kjeldsen H, Borucki WJ, Koch D (2007) Asteroseismology with the Kepler mission. In: Handler G, Houdek G (eds) Proc. Vienna workshop on the future of asteroseismology, Comm. in asteroseismology vol 150, pp 350–356

  • Christy RF (1966). A study of pulsation in RR Lyrae models. Astrophys J 144: 108–179

    Article  ADS  Google Scholar 

  • Claret A (2000). A new non-linear limb-darkening law for LTE stellar atmosphere models. Calculations for  − 0 ≤ log M/H ≤  + 1,2000 K ≤ Teff ≤ 50000 K at several surface gravities. Astron Astrophys 363: 1081–1190

    ADS  Google Scholar 

  • Colavita MM, Wallace JK, Hines BE, Gursel Y, Malbet F, Palmer DL, Pan XP, Shao M, Yu JW, Boden AF, Dumont PJ, Gubler J, Koresko CD, Kulkarni SR, Lane BF, Mobley DW and van Belle GT (1999). The palomar testbed interferometer. Astrophys J 510: 505–521

    Article  ADS  Google Scholar 

  • Colavita MM, Wizinowich PL, Akeson RL (2004) Keck interferometer status and plans. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. of the SPIE, vol 5491, pp 454–463

  • Cox JP (1974). Pulsating stars. Rep Prog Phys 37: 563–698

    Article  ADS  Google Scholar 

  • Cox JP and Giuli RT (1968). Principles of stellar structure. Gordon and Breach, New York

    Google Scholar 

  • Cox JP and Whitney C (1958). Stellar pulsation. IV. A semitheoretical period-luminosity relation for classical Cepheids. Astrophys J 127: 561–572

    Article  ADS  Google Scholar 

  • Creevey OL, Monteiro MJPFG, Metcalfe TM, Brown TM, Jimónez-Reyes SJ and Belmonte JA (2007). The complementary roles of interferometry and asteroseismology in determining the mass of solar-type stars. Astrophys J 659: 616–625

    Article  ADS  Google Scholar 

  • Cunha MS (2001). The sixth frequency of roAp star HR 1217. Mon Not R Astr Soc 325: 373–378

    Article  ADS  Google Scholar 

  • Cunha MS (2002). A theoretical instability strip for rapidly oscillating Ap stars. Mon Not R Astr Soc 333: 47–54

    Article  ADS  Google Scholar 

  • Cunha MS (2005). Asteroseismic theory of rapidly oscillating Ap Stars. J Astrophys Astron 26: 213

    Article  ADS  Google Scholar 

  • Cunha MS (2006). Improved pulsating models of magnetic Ap stars—I. Exploring different magnetic field configurations. Mon Not R Astr Soc 365: 153–164

    Article  ADS  Google Scholar 

  • Cunha MS (2007) Theory of rapidly oscillating Ap stars. In: Handler G, Houdek G (eds) Proc. Vienna workshop on the future of asteroseismology, Comm. in Asteroseismology, vol. 150, pp 48–54

  • Cunha MS and Gough D (2000). Magnetic perturbations to the acoustic modes of roAp stars. Mon Not R Astr Soc 319: 1020–1038

    Article  ADS  Google Scholar 

  • Cunha MS and Metcalfe TS (2007). Asteroseismic signatures of small convective cores: theoretical analysis. Astrophys J 666: 413–422

    Article  ADS  Google Scholar 

  • Cunha MS, Fernandes JMMB and Monteiro MJPFG (2003). Seismic tests of the structure of rapidly oscillating Ap stars: HR 1217. Mon Not R Astr Soc 343: 831–838

    Article  ADS  Google Scholar 

  • Cunha MS, Theádo S, Vauclair S (2004) Excitation of the oscillations in roAp stars: Magnetic fields, diffusion, and winds In: IAU symp. No. 224,The A-Star Puzzle:Cambridge University Press, UK, pp 359–365

  • Cutri RM, Skrutskie MF, Van Dyk S, Beichman CA, Carpenter JM, Chester T, Cambresy L, Evans T, Fowler J, Gizis J, Howard E, Huchra J, Jarrett T, Kopan EL, Kirkpatrick JD, Light RM, Marsh KA, McCallon H, Schneider S, Stiening R, Sykes M, Weinberg M, Wheaton WA, Wheelock S, Zacarias N (2003) 2MASS all sky catalog of point sources. University of Massachusetts and IPAC, http://www.ipac.caltech.edu/2mass.

  • Danchi WC, Bester M, Degiacomi CG, Greenhill LJ and Townes C (1994). Characteristics of dust shells around 13 late-type stars. Astron J 107: 1469–1513

    Article  ADS  Google Scholar 

  • DaszyÅ„ska-Daszkiewicz J, Dziembowski WA, Pamyatnykh AA and Goupil MJ (2002). Photometric amplitudes and phases of nonradial oscillation in rotating stars. Astron Astrophys 392: 151–159

    Article  ADS  Google Scholar 

  • DaszyÅ„ska-Daszkiewicz J, Dziembowski WA, Pamyatnykh AA, Breger M, Zima W and Houdek G (2005). Inferences from pulsational amplitudes and phases for multimode δ Scuti star FG Vir. Astron Astrophys 438: 653–660

    Article  ADS  Google Scholar 

  • DaszyÅ„ska-Daszkiewicz J, Dziembowski WA and Pamyatnykh AA (2006). On the nature of small amplitude peaks in δ Scuti oscillation spectra. Mem Soc Astron Ital 77: 113–116

    ADS  Google Scholar 

  • Davis J, Tango WJ, Booth AJ, ten Brummelaar TA, Minard RA and Owens SM (1999). The Sydney University Stellar Interferometer—I. The instrument. Mon Not Ry Astr Soc 303: 773–782

    Article  ADS  Google Scholar 

  • Davis J, Mendez A, Seneta EB, Tango WJ, Booth AJ, O’Byrne JW, Thorvaldson ED, Ausseloos M, Aerts C and Uytterhoeven K (2005). Orbital parameters, masses and distance to β Centauri determined with the Sydney University Stellar Interferometer and high-resolution spectroscopy. Mon Not Roy Astr Soc 356: 1362–1370

    Article  ADS  Google Scholar 

  • De Cat P and Aerts C (2002). A study of bright southern slowly pulsating B stars. II. The intrinsic frequencies. Astron Astrophys 393: 965–981

    Article  ADS  Google Scholar 

  • De Cat P, Aerts C, De Ridder J, Kolenberg K, Meeus G and Decin L (2000). A study of bright southern slowly pulsating B stars. I. Determination of the orbital parameters and of the main frequency of the spectroscopic binaries. Astron Astrophys 355: 1015–1030

    ADS  Google Scholar 

  • De Cat P, Briquet M, DaszyÅ„ska-Daszkiewicz J, Dupret MA, De Ridder J, Scuflaire R and Aerts C (2005). A study of bright southern slowly pulsating B stars. III. Mode identification for singly-periodic targets in spectroscopy. Astron Astrophys 432: 1013–1024

    Google Scholar 

  • De Cat P, Eyer L, Cuypers J, Aerts C, Vandenbussche B, Uytterhoeven K, Reyniers K, Kolenberg K, Groenewegen M, Raskin G, Maas T and Jankov S (2006). A spectroscopic study of southern (candidate) γ Doradus stars. I. Time series analysis. Astron Astrophys 449: 281–292

    Article  ADS  Google Scholar 

  • De Cat P, Briquet M, Aerts C, Goossens K, Saesen S, Cuypers J, Yakut K, Scuflaire R, Dupret MA, Uytterhoeven K, van Winckel H, Raskin G, Davignon G, Le Guillou L, van Malderen R, Reyniers M, Acke B, de Meester W, Vanautgaerden J, Vandenbussche B, Verhoelst T, Waelkens C, Deroo P, Reyniers K, Ausseloos M, Broeders E, Daszy ska-Daszkiewicz J, Debosscher J, de Ruyter S, Lefever K, Decin G, Kolenberg K, Mazumdar A, van Kerckhoven C, de Ridder J, Drummond R, Barban C, Vanhollebeke E, Maas T and Decin L (2007). Astron Astrophys 463: 243–249

    Article  ADS  Google Scholar 

  • De Ridder J, Dupret MA, Neuforge C and Aerts C (2002). Influence of non-adiabatic temperature variations on line profile variations of slowly rotating β Cep stars and SPBs. II. Simulations of line profile time series. Astron Astrophys 385: 572–584

    Article  ADS  Google Scholar 

  • De Ridder J, Telting JH, Balona LA, Handler G, Briquet M, DaszyÅ„ska-Daszkiewicz J, Lefever K, Korn AJ, Heiter U and Aerts C (2004). Asteroseismology of the β Cephei star ν Eridani—III. Extended frequency analysis and mode identification. Mon Not R ast Soc 351: 324–332

    Google Scholar 

  • Delplancke F, Derie F, Lóvêque S, Mónardi S, Abuter R, Andolfato L, Ballester P, de Jong J, Di Lieto N, Duhoux Ph, Frahm R, Gitton Ph, Glindemann A, Palsa R, Puech F, Sahlmann J, Schuhler N, Duc Th Ph, Valat B, Wallander A (2006) PRIMA for the VLTI: a status report. In: Monnier JD, Schöller M, Danchi WC (eds) Advances in stellar interferometry: Proc. of the SPIE, vol 6268, p 62680U

  • Deubner FL and Gough DO (1984). Helioseismology: oscillations as a diagnostic of the solar interior. Annu Rev Astron Astrophys 22: 593–619

    Article  ADS  Google Scholar 

  • Di Folco E, Thóvenin F, Kervella P, Domiciano de Souza A, Coudó du Foresto V, Sógransan D and Morel P (2004). VLTI near-IR interferometric observations of Vega-like stars. Radius and age of α PsA, β Leo, β Pic, ͛ Eri and τ Cet. Astron Astrophys 426: 601–617

    Google Scholar 

  • Di Mauro MP, Christensen-Dalsgaard J and Paternò L (2003). A Study of the Solar-Like Properties of Hydri. Astrophys Space Sci 284: 229–232

    Article  ADS  Google Scholar 

  • Di Mauro MP, Christensen-Dalsgaard J, Paternó L and D’Antona F (2004). Interpretation of the solar-like pulsational behaviour of η Bootis. Solar Phys 220: 185–198

    Article  ADS  Google Scholar 

  • Domiciano de Souza A, Vakili F, Jankov S, Janot-Pacheco E and Abe L (2002). Modelling rapid rotators for stellar interferometry. Astron Astrophys 393: 345–357

    Article  ADS  Google Scholar 

  • Domiciano de Souza A, Kervella P, Jankov S, Abe L, Vakili F, di Folco E and Paresce F (2003). The spinning-top Be star Achernar from VLTI-VINCI. Astron Astrophys 407: L47–L50

    Article  ADS  Google Scholar 

  • Domiciano de Souza A, Zorec J, Jankov S, Vakili F, Abe L and Janot-Pacheco E (2004). Stellar differential rotation and inclination angle from spectro-interferometry. Astron Astrophys 418: 781–794

    Article  ADS  Google Scholar 

  • Domiciano de Souza A, Kervella P, Jankov S, Vakili F, Ohishi N, Nordgren TE and Abe L (2005). Gravitational-darkening of Altair from interferometry. Astron Astrophys 442: 567–578

    Article  ADS  Google Scholar 

  • Dravins D and Nordlund A (1990a). Stellar Granulation—Part Four—Line Formation in Inhomogeneous Stellar Photospheres. Astron Astrophys 228: 184–202

    ADS  Google Scholar 

  • Dravins D and Nordlund A (1990b). Stellar Granulation—Part Five—Synthetic Spectral Lines in Disk Integrated Starlight. Astron Astrophys 228: 203–217

    ADS  Google Scholar 

  • Dupret MA, De Ridder J, De Cat P, Aerts C, Scuflaire R, Noels A and Thoul A (2003). A photometric mode identification method, including an improved non-adiabatic treatment of the atmosphere. Astron Astrophys 398: 677–685

    Article  ADS  Google Scholar 

  • Dupret MA, Grigahcène A, Garrido R, Gabriel M and Scuflaire R (2004). Theoretical instability strips for δ Scuti and γ Doradus stars. Astron Astrophys 414: L17–L20

    Article  ADS  Google Scholar 

  • Dupret MA, Grigahcène A, Garrido R, Gabriel M and Scuflaire R (2005a). Convection-pulsation coupling. II. Excitation and stabilization mechanisms in δ Scuti and γ Doradus stars. Astron Astrophys 435: 927–939

    Article  ADS  Google Scholar 

  • Dupret MA, Grigahcène A, Garrido R, De Ridder J, Scuflaire R and Gabriel M (2005b). Time-dependent convection seismic study of five γ Doradus stars. Mon Not R Astr Soc 360: 1143–1152

    Article  ADS  Google Scholar 

  • Dupret MA, Grigahcène A, Garrido R, De Ridder J, Scuflaire R and Gabriel M (2005c). Time-dependent convection seismic study of δ Sct stars. Mon Not R Astr Soc 361: 476–486

    Article  ADS  Google Scholar 

  • Duvall TL Jr (1982). A dispersion law for solar oscillations. Nature 300: 242–243

    Article  ADS  Google Scholar 

  • Duvall TL Jr, Dziembowski WA, Goode PR, Gough DO, Harvey JW and Leibacher JW (1982). Internal rotation of the sun. Nature 310: 22–25

    Article  ADS  Google Scholar 

  • Dyck HM (2000). Interferometry with Two Telescopes. In: Lawson, PR (eds) Principles of long baseline stellar interferometry, pp 185–202. Published by NASA, JPL, CIT, Pasadena

    Google Scholar 

  • Dziembowski WA (1977). Light and radial velocity variations in a nonradially oscillating star. Acta Astron 27: 203–211

    ADS  Google Scholar 

  • Dziembowski WA and Goode PR (1992). Effects of differential rotation on stellar oscillations: a second-order theory. Astrophys J 394: 670–687

    Article  ADS  Google Scholar 

  • Dziembowski WA and Goode PR (1996). Magnetic effects on oscillations in roAp stars. Astrophys J 458: 338–346

    Article  ADS  Google Scholar 

  • Dziembowski W and Królikowska M (1985). Nonlinear mode coupling in oscillating stars. II. Limiting amplitude effect of the parametric resonance in main sequence stars. Acta Astron 35: 5–28

    ADS  Google Scholar 

  • Dziembowski WA, Gough DO, Houdek G and Sienkiewicz R (2001). Oscillations of α UMa and other red giants. Mon Not R Astr Soc 328: 601–610

    Article  ADS  Google Scholar 

  • Eddington AS (1926). The internal constitution of the stars. Cambridge University Press, Cambridge

    MATH  Google Scholar 

  • Edmonds PD and Cram LE (1995). A search for global acoustic oscillations on α1 Cen and β Hyi. Mon Not R Astr Soc 276: 1295–1302

    ADS  Google Scholar 

  • Eggenberger P, Charbonnel C, Talon S, Meynet G, Maeder A, Carrier F and Bourban G (2004). Analysis of α Centauri AB including seismic constraints. Astron Astrophys 417: 235–246

    Article  ADS  Google Scholar 

  • Eisner JA, Graham JR, Akeson RL, Ligon ER, Colavita MM, Basri G, Summers K, Ragland S and Booth A (2007). Stellar and molecular radii of a Mira star: first observations with the Keck interferometer grism. Astrophys J 654: L77–L80

    Article  ADS  Google Scholar 

  • Ellis AN (1984) The base of the solar convection zone. In: Theoretical problems in stellar stability and oscillations, Institute d’Astrophysique, Liège, pp 298–301

  • Ellis AN (1986). An improved asymptotic formula for solar gravity-mode periods. In: Gough, DO (eds) Seismology of the Sun and the distant stars, pp 173–175. Reidel, Dordrecht

    Google Scholar 

  • Fernandes J and Monteiro MJPFG (2003). HR diagram and asteroseismic analysis of models for beta Hydri. Astron Astrophys 399: 243–251

    Article  ADS  Google Scholar 

  • Feuchtinger MU (1999). A nonlinear convective model for radial stellar pulsations. I. The physical description. Astron Astrophys Suppl 136: 217–226

    Article  ADS  Google Scholar 

  • Fletcher ST, Chaplin WJ, Elsworth Y, Schou J and Buzasi D (2006). Frequency, splitting, linewidth and amplitude estimates of low-â„“ p modes of α Cen A: analysis of wide-field infrared explorer photometry. Mon Not R Astr Soc 371: 935–944

    Article  ADS  Google Scholar 

  • Fontaine G, Brassard P (2005) Asteroseismology of the crystallized ZZ ceti Star BPM 37093: a different view (Part II). In: Koester D, Moehler S (eds) 14th European Workshop on White Dwarfs. ASP Conference Series, vol 334, p 565

  • Fontaine G, Brassard P, Charpinet S, Green EM, Chayer P, Billères M and Randall SK (2003). A driving mechanism for the newly discovered long-period pulsating subdwarf B stars. Astrophys J 597: 518–534

    Article  ADS  Google Scholar 

  • Frandsen S (1987). An upper limit on p-mode amplitudes in β Hyi. Astron Astrophys 181: 289–292

    ADS  Google Scholar 

  • Frandsen S, Carrier F, Aerts C, Stello D, Maas T, Burnet M, Bruntt H, Teixeira TC, de Medeiros JR, Bouchy F, Kjeldsen H, Pijpers F and Christensen-Dalsgaard J (2002). Detection of solar-like oscillations in the G7 giant star ξ Hya. Astron Astrophys 394: L5–L8

    Article  ADS  Google Scholar 

  • Frazier EN (1968). A spatio-temporal analysis of velocity fields in the solar photosphere. Zeitschrift fr Astrophysik 68: 345–356

    ADS  Google Scholar 

  • Gabriel M (1996). Solar oscillations: theory. Bull Astr Soc India 24: 233–243

    ADS  Google Scholar 

  • Gabriel M (2000). Linear interaction between pulsations and convection, scattering and line profiles of solar p-modes. Astron Astrophys 353: 399–408

    ADS  Google Scholar 

  • Gabriel M, Scuflaire R, Noels A and Boury A (1974). Influence de la convection sur la stabilitó des oscillations non radiales des ótoiles. Bull Acad R Belg Classe des Sc, 5e Sórie 60: 866–887

    Google Scholar 

  • Gabriel M, Scuflaire R, Noels A and Boury A (1975). Influence of convection on the vibrational stability of stars towards non-radial oscillations. Astron Astrophys 40: 33–39

    ADS  Google Scholar 

  • García RA, Rógulo C, Turck-Chièze S, Bertello L, Kosovichev AG, Brun AS, Couvidat S, Henney CJ, Lazrek M, Ulrich RK and Varadi F (2001). Low-degree low-order solar p modes as seen by GOLF on board SOHO. Solar Phys 200: 361–379

    Article  ADS  Google Scholar 

  • Garrido R (2000) Photometric modal discrimination in δ Scuti and γ Doradus stars. In: Breger M, Montgomery MH (eds) Delta Scuti and related stars, ASP Conference Series, vol 210, San Francisco, pp 67–98

  • Gehmeyr M (1993). On nonlinear radial oscillations in convective RR Lyrae stars. III. A full-amplitude investigation of the red edge. Astrophys J 412: 341–350

    Google Scholar 

  • Gehmeyr M and Winkler KHA (1992). On a new one-dimensional, time-dependent model for turbulence and convection. I. A basic discussion of the mathematical model. Astron Astrophys 253: 92–100

    MATH  ADS  MathSciNet  Google Scholar 

  • Gies DR and Kullavanijaya A (1988). The line profile variations of Epsilon Persei. I - Evidence for multimode nonradial pulsations. Astrophys J 326: 813–831

    Article  ADS  Google Scholar 

  • Gillessen S, Perrin G, Brandner W, Straubmeier C, Eisenhauer F, Rabien S, Eckart A, Lena P, Genzel R, Paumard T, Hippler S (2006) GRAVITY: the adaptive-optics-assisted two-object beam combiner instrument for the VLTI. In: Monnier JD, Schöller M, Danchi WC (eds) Advances in stellar interferometry, Proc. SPIE vol 6268, p 626811

  • Gilliland RL, Brown TM, Kjeldsen H, McCarthy JK, Peri ML, Belmonte JA, Vidal I, Cram LE, Palmer J, Frandsen S, Parthasarathy M, Petro L, Schneider H, Stetson PB and Weiss WW (1993). A search for solar-like oscillations in the stars of M67 with CCD ensemble photometry on a network of 4 m telescopes. Astron J 106: 2441–2476

    Article  ADS  Google Scholar 

  • Gizon L and Solanki S (2003). Determining the inclination of the rotation axis of a Sun-like star. Astrophys J 589: 1009–1019

    Article  ADS  Google Scholar 

  • Gizon L and Solanki S (2004). Measuring stellar differential rotation with asteroseismology. Solar Phys 220: 169–184

    Article  ADS  Google Scholar 

  • Glindemann A, Abuter R, Carbognani F, Delplancke F, Derie F, Gennai A, Gitton PB, Kervella P, Koehler B, Leveque SA, Menardi S, Michel A, Paresce F, Duc, Th. P., Richichi A, Schoeller M, Tarenghi M, Wallander A, Wilhelm R (2000) The VLT interferometer: a unique instrument for high-resolution astronomy. In: Lóna PJ, Quirrenbach A (eds) Interferometry in optical astronomy, Proc. SPIE, 4006, pp 2–12

  • Glindemann A, Albertsen M, Avila G, Ballester P, Bauvir B, Delplancke F, Derie F, et al. (2004) VLTI technical advances: present and future. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. SPIE, 5491, p 447

  • Goldreich P and Keeley DA (1977). Solar seismology. II. The stochastic excitation of the solar p-modes by turbulent convection. Astrophys J 212: 243–251

    Article  ADS  Google Scholar 

  • Goldreich P and Wu Y (1999). Gravity modes in ZZ Ceti stars. I. Quasi-adiabatic analysis of overstability. Astrophys J 511: 904–915

    Article  ADS  Google Scholar 

  • Gonczi G (1981). On local theories of time dependent convection in the stellar pulsation problem. Astron Astrophys 96: 138–141

    ADS  Google Scholar 

  • Goodman JW (1985). Statistical Optics. Wiley, New York

    Google Scholar 

  • Gough DO (1977a). Random remarks on solar hydrodynamics. In: Bonnet, RM and Delache, Ph (eds) The energy balance and hydrodynamics of the solar chromosphere and corona, pp 3–36. G.de Bussac, Clermont-Ferrand

    Google Scholar 

  • Gough DO (1977b). Mixing-length theory for pulsating stars. Astrophys J 214: 196–213

    Article  ADS  Google Scholar 

  • Gough DO (1977c). The current state of stellar mixing-length theory. In: Spiegel, EA and Zahn, JP (eds) Problems of stellar convection, IAU Colloq. No. 38, Lecture notes in physics vol 71, pp 15–56. Springer, Berlin

    Google Scholar 

  • Gough DO (1978) The significance of solar oscillations. In: Pleins feux sur la physique solaire. Proc. 2me Assemblóe Europóenne de Physique Solaire. CNRS, Paris, pp 81–103

  • Gough DO (1981). A new measure of the solar rotation. Mon Not R Astr Soc 196: 731–745

    ADS  Google Scholar 

  • Gough DO (1985a) Theory of solar oscillations. In: Rolfe E, Battrick B (eds) Future missions in solar, heliospheric and space plasma physics, ESA SP-235, ESTEC, Noordwijk, pp 183–197

  • Gough DO (1985b). Inverting helioseismic data. Solar Phys 100: 65–99

    Article  ADS  Google Scholar 

  • Gough DO (1986). EBK quantization of stellar waves. In: Osaki, Y (eds) Hydrodynamic and magnetohydrodynamic problems in the Sun and stars, Department of Astronomy, pp 117–143. University of Tokyo, Tokyo

    Google Scholar 

  • Gough DO (1987). Seismological measurement of stellar ages. Nature 326: 257–259

    Article  ADS  Google Scholar 

  • Gough DO (1993). Course 7. In: Linear adiabatics tellar pulsation. Zahn, JP and Zinn-Justin, J (eds) Astrophysical fluid dynamics, Les Houches Session XLVII, pp 399–560. Elsevier, Amsterdam

    Google Scholar 

  • Gough DO and Kosovichev AG (1990). Using helioseismic data to probe the hydrogen abundance in the solar core. In: Berthomieu, G and Cribier, M (eds) Proc. IAU Colloquium No 121, Inside the Sun, pp 327–340. Kluwer, Dordrecht

    Google Scholar 

  • Gough DO and Thompson MJ (1990). The effect of rotation and a buried magnetic field on stellar oscillations. Mon Not R Astr Soc 242: 25–55

    MATH  ADS  Google Scholar 

  • Gough DO, Kosovichev AG, Toomre J, Anderson ER, Antia HM, Basu S, Chaboyer B, Chitre SM, Christensen-Dalsgaard J, Dziembowski WA, Eff-Darwich A, Elliott JR, Giles PM, Goode PR, Guzik JA, Harvey JW, Hill F, Leibacher JW, Monteiro MJPFG, Richard O, Sekii T, Shibahashi H, Takata M, Thompson MJ, Vauclair S and Vorontsov SV (1996). The seismic structure of the Sun. Science 272: 1296–1300

    Article  ADS  Google Scholar 

  • Goupil MJ, Samadi R, Lochard J, Dziembowski WA and Pamyatnykh A (2004). Inferring information about rotation from stellar oscillations. In: Favata, F and Aigrain, S (eds) Proc. 2nd Eddington workshop, stellar structure and habitable planet finding, ESA SP-538, pp 133–140. ESA Publications Division, Noordwijk, The Netherlands

    Google Scholar 

  • Gray DF (1977). A quest for differential stellar rotation in A stars. Astrophys J 211: 198–206

    Article  ADS  Google Scholar 

  • Grec G, Fossat E and Pomerantz M (1980). Solar oscillations: full disk observations from the geographic South Pole. Nature 288: 541–544

    Article  ADS  Google Scholar 

  • Grigahcène A, Dupret MA, Gabriel M, Garrido R and Scuflaire R (2005). Convection-pulsation coupling. I. A mixing-length perturbative theory. Astron Astrophys 434: 1055–1062

    Article  ADS  Google Scholar 

  • Grundahl F, Kjeldsen H, Christensen-Dalsgaard J, Arentoft T, Frandsen S (2007) Stellar oscillations network group. In: Handler G, Houdek G (eds) Proc. Vienna workshop on the future of Asteroseismology, Comm. in asteroseismology, vol 150, pp 300–306

  • Guenther DB (2004). Quantitative analysis of the oscillation spectrum of η Bootis. Astrophys J 612: 454–462

    Article  ADS  Google Scholar 

  • Guenther DB and Brown KIT (2004). Matching stellar models to oscillation data. Astrophys J 600: 419–434

    Article  ADS  Google Scholar 

  • Guenther DB and Demarque P (1996). Seismology of η Bootis. Astrophys J 456: 798–810

    Article  ADS  Google Scholar 

  • Guzik JA (2006). Reconciling the revised solar abundances with helioseismic constraints. In: Fletcher, K (eds) Proc. SOHO 18 / GONG 2006 / HELAS I Conf. beyond the spherical Sun, ESA SP-624, ESA Publications Division, pp 1–11. Noordwijk, The Netherlands

    Google Scholar 

  • Guzik JA, Kaye AB, Bradley PA, Cox AN and Neuforge C (2000). Driving the gravity-mode pulsations in γ Doradus variables. Astrophys J 542: L57–L60

    Article  ADS  Google Scholar 

  • Hajian AR, Armstrong JT, Hummel CA, Benson JA, Mozurkewich D, Pauls TA, Hutter DJ, Elias NM, Johnston KJ, Rickard LJ and White NM (1998). Direct confirmation of stellar limb darkening with the Navy Prototype Optical Interferometer. Astrophys J 496: 484–489

    Article  ADS  Google Scholar 

  • Hale DDS, Weiner J, Townes CH (2004) ISI: recent technology and science. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. SPIE 5491, pp 490–498

  • Hanbury Brown R, Davis J and Allen R (1974a). The angular diameters of 32 stars. Mon Not R Astr Soc 167: 121–136

    ADS  Google Scholar 

  • Hanbury Brown R, Davis J, Lake RJW and Thompson RJ (1974b). The effects of limb darkening on measurements of angular size with an intensity interferometer. Mon Not R Astr Soc 167: 475–484

    ADS  Google Scholar 

  • Handler G, Arentoft T, Shobbrook RR, Wood MA, Crause LA, Crake P, Podmore F, Habanyama A, Oswalt T, Birch PV, Lowe G, Sterken C, Meintjes P, Brink J, Claver CF, Medupe R, Guzik JA, Beach TE, Martinez P, Leibowitz EM, Ibbetson PA, Smith T, Ashoka BN, Raj NE, Kurtz DW, Balona LA, O’Donoghue D, Costa JES and Breger M (2000). Delta Scuti Network observations of XX Pyx: detection of 22 pulsation modes and of short-term amplitude and frequency variations. Mon Not R Astr Soc 318: 511–525

    Article  ADS  Google Scholar 

  • Handler G, Shobbrook RR, Vuthela FF, Balona LA, Rodler F and Tshenye T (2003). Asteroseismological studies of three ? Cephei stars: IL Vel, V433 Car and KZ Mus. Mon Not R Astr Soc 341: 1005–1019

    Article  ADS  Google Scholar 

  • Handler G, Shobbrook RR, Jerzykiewicz M, Krisciunas K, Tshenye T, Rodríguez E, Costa V, Zhou AY, Medupe R, Phorah WM, Garrido R, Paparó M, Zsuffa D, Ramokgali L, Crowe R, Purves N, Avila R, Knight R, Brassfield E, Kilmartin PM and Cottrell PL (2004). Asteroseismology of the β Cephei star ν Eridani—I. Photometric observations and pulsational frequency analysis. Mon Not R Astr Soc 347: 454–462

    Article  ADS  Google Scholar 

  • Handler G, Shobbrook RR and Mokgwetsi T (2005). An asteroseismic study of the β Cepehi star θ Ophiuchi: photometric results. Mon Not R Astr Soc 362: 612–618

    Article  ADS  Google Scholar 

  • Handler G, Jerzykiewicz M, Rodríguez E, Uytterhoeven K, Amado PJ, Dorokhova TN, Dorokhov NI, Poretti E, Sareyan JP, Parrao L, Lorenz D, Zsuffa D, Drummond R, DaszyÅ„ska-Daszkiewicz J, Verhoelst T, De Ridder J, Acke B, Bourge PO, Movchan AI, Garrido R, Paparó M, Sahin T, Antoci V, Udovichenko SN, Csorba K, Crowe R, Berkey B, Stewart S, Terry D, Mkrtichian DE and Aerts C (2006). Asteroseismology of the β Cephei star 12 (DD) Lacertae: photometric observations, pulsational frequency analysis and mode identification. Mon Not R Astr Soc 365: 327–338

    Article  ADS  Google Scholar 

  • Hansen CJ, Cox JP and van Horn HM (1977). The effects of differential rotation on the splitting of nonradial modes of stellar oscillation. Astrophys J 217: 151–159

    Article  ADS  Google Scholar 

  • Hao J (1998). Line profile analysis of nonradial pulsation modes based on Doppler imaging. Astrophys J 500: 440–448

    Article  ADS  Google Scholar 

  • Hauschildt PH, Allard F, Ferguson J, Baron E and Alexander DR (1999). The NEXTGEN model atmosphere grid. II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800 K. Astrophys J 525: 871–880

    Article  ADS  Google Scholar 

  • Hekker S, Caerts C, De Ridder J and Carrier F (2006). Pulsations detected in the line profile variations of red giants. Modelling of line moments, line bisector and line shape. Astron Astrophys 458: 931–940

    Google Scholar 

  • Henyey LG, Vardya MS and Bodenheimer P (1965). Studies in stellar evolution. III. The calculation of model envelopes. Astrophys J 142: 841–854

    Article  ADS  Google Scholar 

  • Herbison-Evans D, Hanbury Brown R, Davis J and Allen LR (1971). A study of α Virginis with an intensity interferometer. Mon Not Roy Astr Soc 151: 161–176

    ADS  Google Scholar 

  • Heynderickx D, Waelkens C and Smeyers P (1994). A photometric study of β Cephei stars. II. Determination of the degrees L of pulsation modes. Astron Astrophys Suppl 105: 447–480

    ADS  Google Scholar 

  • Hoffleit D (1997). History of the discovery of Mira stars. JAVSO 25: 115–136

    ADS  Google Scholar 

  • Houdek G (2000) Convective effects on p-mode stability in Delta Scuti stars. In: Breger M, Montgomery MH (eds) Delta Scuti and related stars, ASP Conference Series, vol 210, San Francisco, pp 454–463

  • Houdek G (2002) Stochastic excitation in solar-type stars. In: Aerts C, Bedding TR, Christensen-Dalsgaard J (eds) Proc. IAU Colloq. 185: Radial and nonradial pulsations as probes of stellar physics, ASP Conference Series, vol 259, pp 447–455

  • Houdek G (2004) Asteroseismic helium abundance determination. In: ÄŒelebonovi´c V, Däppen W, Gough D (eds) Equation-of-state and phase-transition issues in models of ordinary astrophysical matter, AIP Conference Proceedings vol 731, AIP, Melville, New York, pp 193–207

  • Houdek G (2006). Stochastic excitation and damping of solar-type oscillations. In: Fletcher, K (eds) Proc. SOHO 18 / GONG 2006 / HELAS I Conf. Beyond the spherical Sun, ESA SP-624, pp 1–12. ESA Publications Division, Noordwijk

    Google Scholar 

  • Houdek G and Gough DO (2002). Modelling pulsation amplitudes of ξ Hydrae. Mon Not R Astr Soc 336: L65–L69

    Article  ADS  Google Scholar 

  • Houdek G, Gough DO (2006) On seismic signatures of rapid variation. In: Fletcher K (ed) Proc. SOHO 18 / GONG 2006 / HELAS I Conference Beyond the spherical Sun, ESA SP-624, ESA Publications Division, Noordwijk pp 1–6

  • Houdek G and Gough DO (2007). An asteroseismic signature of helium ionization. Mon Not R Astr Soc 375: 861–880

    Article  ADS  Google Scholar 

  • Houdek G, Balmforth NJ, Christensen-Dalsgaard J and Gough DO (1999). Amplitudes of stochastically excited oscillations in main-sequence stars. Astron Astrophys 351: 582–596

    ADS  Google Scholar 

  • Hummel CA, Armstrong JT, Quirrenbach A, Buscher DF, Mozurkewich D, Simon RS and Johnston KJ (1993). The spectroscopic binary η Andromedae: determination of the orbit by optical interferometry. Astron J 106: 2486–2492

    Article  ADS  Google Scholar 

  • Hummel CA, Armstrong JT, Quirrenbach A, Buscher DF, Mozurkewich D, Elias NM and Wilson RE (1994). Very high precision orbit of Capella by long baseline interferometry. Astron J 107: 1859–1867

    Article  ADS  Google Scholar 

  • Hummel CA, Armstrong JT, Buscher DF, Mozurkewich D, Quirrenbach A and Vivekanand M (1995). Orbits of small angular scale binaries resolved with the Mark III interferometer. Astron J 110: 376–390

    Article  ADS  Google Scholar 

  • Hummel CA, Mozurkewich D, Armstrong JT, Hajian AR, Elias NM and Hutter DJ (1998). Navy Prototype Optical Interferometer Observations of the Double Stars Mizar A and Matar. Astron J 116: 2536–2548

    Article  ADS  Google Scholar 

  • Hummel CA, Carquillat JM, Ginestet N, Griffin RF, Boden AF, Hajian AR, Mozurkewich D and Nordgren TE (2001). Orbital and stellar parameters of Omicron Leonis from spectroscopy and interferometry. Astron J 121: 1623–1635

    Article  ADS  Google Scholar 

  • Hummel CA, Benson JA, Hutter DJ, Johnston KJ, Mozurkewich D, Armstrong JT, Hindsley RB, Gilbreath GC, Rickard LJ and White NM (2003). First observations with a co-phased six-station optical long-baseline array: application to the triple star η Virginis. Astron J 125: 2630–2644

    Article  ADS  Google Scholar 

  • Jackson S, MacGregor KB and Skumanich A (2005). On the use of the self-consistent-field method in the construction of models for rapidly rotating main-sequence stars. Astrophys J Suppl 156: 245–264

    Article  ADS  Google Scholar 

  • Jankov S, Vakili F, Domicianode Souza A Jr and Janot-Pacheco E (2001a). Interferometric-Doppler imaging of stellar surface structure. Astron Astrophys 377: 721–734

    Article  ADS  Google Scholar 

  • Jankov S, Vakili F, Domiciano de Souza A Jr, Janot-Pacheco E (2001b) Interferometric-Doppler Imaging of Nonradial Stellar Pulsations. In: Aerts C, Bedding TR, Christensen-Dalsgaard J (eds) Radial and nonradial pulsations as probes of stellar physics, ASP Conference Series, vol 259, pp 172–175

  • Jankov S, Mathias P, Domiciano de Souza A Jr, Uytterhoeven K, Aerts C (2004) Latitude distribution of nonradial pulsations in rapidly rotating B stars. In: Variable Stars in the Local Group, ASP Conference Series, vol 310, pp 204–207

  • Jeffery CS, Aerts C, Dhillon VS, Marsh TR and Gänsicke BT (2005). Multicolour high-speed photometry of the subdwarf B star PG 0014+067 with ULTRACAM. Mon Not R Astr Soc 362: 66–78

    Article  ADS  Google Scholar 

  • Jeffery CS, Dhillon VS, Marsh TR and Ramachandran B (2004). Multicolour high-speed photometry of pulsating subdwarf B stars with ULTRACAM. Mon Not R Astr Soc 352: 699–707

    Article  ADS  Google Scholar 

  • Kanaan A, Nitta A, Winget DE, Kepler SO, Montgomery MH, Metcalfe TS, Oliveira H, Fraga L, da Costa AFM, Costa JES, Castanheira BG, Giovannini O, Nather RE, Mukadam A, Kawaler SD, O’Brien MS, Reed MD, Kleinman SJ, Provencal JL, Watson TK, Kilkenny D, Sullivan DJ, Sullivan T, Shobbrook B, Jiang XJ, Ashoka BN, Seetha S, Leibowitz E, Ibbetson P, Mendelson H, Meištas EG, Kalytis R, Ališauskas D, O’Donoghue D, Buckley D, Martinez P, van Wyk F, Stobie R, Marang F, van Zyl L, Ogloza W, Krzesinski J, Zola S, Moskalik P, Breger M, Stankov A, Silvotti R, Piccioni A, Vauclair G, Dolez N, Chevreton M, Deetjen J, Dreizler S, Schuh S, Gonzalez Perez JM, Østensen R, Ulla A, Manteiga M, Suarez O, Burleigh MR and Barstow MA (2005). Whole Earth Telescope observations of BPM 37093: A seismological test of crystallization theory in white dwarfs. Astron Astrophys 432: 219–224

    Article  ADS  Google Scholar 

  • Kaye AB, Handler G, Krisciunas K, Poretti E and Zerbi FM (1999). Gamma doradus stars: defining a new class of pulsating variables. Publ Astron Soc Pacific 111: 840–844

    Article  ADS  Google Scholar 

  • Kennelly EJ, Walker GAH (1996a) Publ Astron Soc Pacific 108:327–331

    Google Scholar 

  • Kennelly EJ, Walker GAH, Catala C, Foing BH, Huang L, Jiang S, Hao J, Zhai D, Zhao F, Neff JE, Houdebine ER, Ghosh KK and Charbonneau P (1996b). The oscillation modes of θ2 Tauri. Results from the 1992 MUSICOS campaign. Astron Astrophys 313: 571–580

    ADS  Google Scholar 

  • Kepler SO (2007). Observational white dwarf seismology. CoAst 150: 221–226

    ADS  Google Scholar 

  • Kervella P and Domicianode Souza A (2006). The polar wind of the fast rotating Be star Achernar. VINCI/VLTI interferometric observations of an elongated polar envelope. Astron Astrophys 453: 1059–1066

    Article  ADS  Google Scholar 

  • Kervella P, Gitton Ph, Ségransan D, di Folco E, Kern PY, Kiekebusch M, Duc TP, Longinotti A, Coude du Foresto V, Ballester P, Sabet C, Cotton, William D., Schoeller M, Wilhelm R (2003a) VINCI, the VLTI commissioning instrument: status after one year of operations at Paranal. In: Traub WA (ed) Interferometry for optical astronomy II, Proc. SPIE 4838, pp 858–869

  • Kervella P, Thévenin F, Ségransan D, Berthomieu G, Lopez B, Morel P and Provost J (2003b). The diameters of α Centauri A and B. A comparison of the asteroseismic and VINCI/VLTI views. Astron Astrophys 404: 1087–1097

    Article  ADS  Google Scholar 

  • Kervella P, Nardetto N, Bersier D, Mourard D and Coudédu Foresto V (2004a). Cepheid distances from infrared long-baseline interferometry. I. VINCI/VLTI observations of seven galactic cepheids. Astron Astroph 416: 941–953

    Article  ADS  Google Scholar 

  • Kervella P, Thévenin F, Di Folco E and Ségransan D (2004b). The angular sizes of dwarf stars and subgiants. Surface brightness relations calibrated by interferometry. Astron Astrophys 426: 297–307

    Article  ADS  Google Scholar 

  • Kervella P, Thévenin F, Morel P, Berthomieu G, Bordé P and Provost J (2004c). The diameter and evolutionary state of Procyon A. Multi-technique modeling using asteroseismic and interferometric constraints. Astron Astrophys 413: 251–256

    Article  ADS  Google Scholar 

  • Kilkenny D, Reed MD, O’Donoghue D, Kawaler SD, Mukadam A, Kleinman SJ, Nitta A, Metcalfe TS, Provencal JL, Watson TK, Sullivan DJ, Sullivan T, Shobbrook R, Jiang XJ, Joshi S, Ashoka BN, Seetha S, Leibowitz E, Ibbetson P, Mendelson H, MeiÅ¡tas E, Kalytis R, AliÅ¡auskas D, Martinez P, van Wyk F, Stobie RS, Marang F, Zola S, Krzesinski J, Ogloza W, Moskalik P, Silvotti R, Piccioni A, Vauclair G, Dolez N, Chevreton M, Dreizler S, Schuh SL, Deetjen JL, Solheim JE, Gonzalez Perez JM, Ulla A, Østensen R, Manteiga M, Suarez O, Burleigh M, Kepler SO, Kanaan A and Giovannini O (2003). A Whole Earth Telescope campaign on the pulsating subdwarf B binary system PG 1336–018 (NY Vir). Mon Not R Astr Soc 345: 834–846

    Article  ADS  Google Scholar 

  • Kjeldsen H and Bedding TR (1995). Amplitudes of stellar oscillations: the implications for asteroseismology. Astron Astrophys 293: 87–106

    ADS  Google Scholar 

  • Kjeldsen H, Bedding TR, Viskum M and Frandsen S (1995). Solarlike oscillations in η Boo. Astron J 109: 1313–1319

    Article  ADS  Google Scholar 

  • Kjeldsen H, Bedding TR, Baldry IK, Bruntt H, Butler RP, Fischer DA, Frandsen S, Gates EL, Grundahl F, Lang K, Marcy GW, Misch A and Vogt SS (2003). Confirmation of solar-like oscillations in η Bootis. Astron J 126: 1483–1488

    Article  ADS  Google Scholar 

  • Kjeldsen H, Bedding TR, Butler RP, Christensen-Dalsgaard J, Kiss LL, McCarthy C, Marcy GW, Tinney CG and Wright JT (2005). Solar-like oscillations in α Centauri B. Astrophys J 635: 1281–1290

    Article  ADS  Google Scholar 

  • Kochukhov O (2004). Indirect imaging of nonradial pulsations in a rapidly oscillating Ap Star. Astrophys J 615: L149–L152

    Article  ADS  Google Scholar 

  • Kochukhov O, Drake NA, Piskunov N and de la Reza R (2004). Multi-element abundance Doppler imaging of the rapidly oscillating Ap star HR 3831. Astron Astrophys 424: 935–950

    Article  ADS  Google Scholar 

  • Koen C (1999). The analysis of indexed astronomical time series - V. Fitting sinusoids to high-speed photometry. Mon Not R Astr Soc 309: 769–802

    Article  ADS  Google Scholar 

  • Koen C and Lombard F (1995). The analysis of indexed astronomical time series - III. Intrinsic period scatter. Mon Not R Astr Soc 274: 821–831

    ADS  Google Scholar 

  • Konacki M and Lane BF (2004). The visual orbits of the spectroscopic binaries HD 6118 and HD 27483 from the Palomar Testbed Interferometer. Astrophys J 610: 443–455

    Article  ADS  Google Scholar 

  • Kosovichev AG (1995) The upper convective boundary layer. In: Hoeksema JT, Domingo V, Fleck B, Battrick B (eds) Proc. Fourth SOHO Workshop: Helioseismology. ESA SP-376, vol 1, ESTEC, Noordwijk, pp 165–176

  • Kosovichev AG, Schou J, Scherrer PH, Bogart RS, Bush RI, Hoeksema JT, Aloise J, Bacon L, Burnette A, de Forest C, Giles PM, Leibrand K, Nigam R, Rubin M, Scott K, Williams SD, Basu S, Christensen-Dalsgaard J, Däppen W, Rhodes EJ Jr, Duvall TL Jr, Howe R, Thompson MJ, Gough DO, Sekii T, Toomre J, Tarbell TD, Title AM, Mathur D, Morrison M, Saba JLR, Wolfson CJ, Zayer I and Milford PN (1997). Structure and rotation of the solar interior: initial results from the MDI medium-l program. Solar Phys 170: 43–61

    Article  ADS  Google Scholar 

  • Kraus S, Balega YY, Berger JP, Hofmann KH, Millan-Gabet R, Monnier JD, Ohnaka K, Pedretti E, Preibisch Th, Schertl D, Schloerb FP, Traub WA and Weigelt G (2007). Visual/infrared interferometry of Orion Trapezium stars: preliminary dynamical orbit and aperture synthesis imaging of the θ1 Orionis C system. Astron Astrophys 466: 649–659

    Article  ADS  Google Scholar 

  • Kuhfuß R (1986). A model of time-dependent turbulent convection. Astron Astrophys 160: 116–120

    ADS  Google Scholar 

  • Kurtz DW (2002) Meeting summary and outlook for the future. In: Aerts C, Bedding TR, Christensen-Dalsgaard J (eds) Radial and nonradial pulsations as probes of stellar physics. ASP Conference Series, vol 259, 639–667

  • Kurtz DW, Kawaler SD, Riddle RL, Reed MD, Cunha MS, Wood M, Silvestri N, Watson TK, Dolez N, Moskalik P, Zola S, Pallier E, Guzik JA, Metcalfe TS, Mukadam AS, Nather RE, Winget DE, Sullivan DJ, Sullivan T, Sekiguchi K, Jiang X, Shobbrook R, Ashoka BN, Seetha S, Joshi S, O’Donoghue D, Handler G, Mueller M, Gonzalez Perez JM, Solheim JE, Johannessen F, Ulla A, Kepler SO, Kanaan A, da Costa A, Fraga L, Giovannini O and Matthews JM (2002). Discovery of the ‘missing’ mode in HR1217 by the Whole Earth Telescope. Mon Not R Astr Soc 330: L57–L61

    Article  ADS  Google Scholar 

  • Kurtz DW, Elkin VG, Mathys G, Riley J, Cunha MS, Shibahashi H and Kambe E (2004). Some recent discoveries in roAp stars. In: Zverko, J, Ziznovsky, J, Adelman, SJ, and Weiss, WW (eds) The A-Star puzzle, IAU symposium, No 224, pp 343–352. Cambridge University Press, Cambridge

    Google Scholar 

  • Kurtz DW, Cameron C, Cunha MS, Dolez N, Vauclair G, Pallier E, Ulla A, Kepler SO, da Costa A, Kanaan A, Fraga L, Giovannini O, Wood MA, Silvestri N, Kawaler SD, Riddle RL, Reed MD, Watson TK, Metcalfe TS, Mukadam A, Nather RE, Winget DE, Nitta A, Kleinman SJ, Guzik JA, Bradley PA, Matthews JM, Sekiguchi K, Sullivan DJ, Sullivan T, Shobbrook R, Jiang X, Birch PV, Ashoka BN, Seetha S, Girish V, Joshi S, Moskalik P, Zola S, O’Donoghue D, Handler G, Mueller M, Gonzalez Perez JM, Solheim JE, Johannessen F and Bigot L (2005). Pushing the ground-based limit: 14-μmag photometric precision with the definitive Whole Earth Telescope asteroseismic data set for the rapidly oscillating Ap star HR 1217. Mon Not R Astr Soc 358: 651–664

    Article  ADS  Google Scholar 

  • Kurucz RL (1992). Model atmospheres for population synthesis. In: Barbuy, B and Renzini, A (eds) Proc. IAU symposium No 149: the stellar populations of galaxies, pp 225–232. Kluwer, Dordrecht

    Google Scholar 

  • Lamb H (1909). On the theory of waves propagated vertically in the atmosphere. Proc London Math Soc 7: 122–141

    Article  Google Scholar 

  • Lane BF, Kuchner MJ, Boden AF, Creech-Eakman M and Kulkarni SR (2000). Direct detection of pulsations of the Cepheid star ζ Gem and an independent calibration of the period-luminosity relation. Nature 407: 485–487

    Article  ADS  Google Scholar 

  • Lane BF, Boden AF and Kulkarni SR (2001). Interferometric measurement of the angular sizes of dwarf stars in the spectral range K3-M4. Astrophys J 551: L81–L83

    Article  ADS  Google Scholar 

  • Lardière O, Martinache F and Patru F (2007). Direct imaging with highly diluted apertures - I. Field-of-view limitations. Mon Not R Astr Soc 375: 977–988

    Article  ADS  Google Scholar 

  • Lawson, Peter R (2000) Principles of long baseline stellar interferometry. In: Lawson PR (ed) Course notes from the 1999 Michelson Summer School, held August 15–19, 1999, National Aeronautics and Space Administration, Jet Propulsion Laboratory, Passadena

  • Leavitt HS (1908). 1777 Variables in the magellanic clouds. Ann Harvard College Observ 60: 87–108

    ADS  Google Scholar 

  • Leccia S, Kjeldsen H, Bonanno A, Claudi RU, Ventura R and Paternó L (2007). Seismology of Procyon A: determination of mode frequencies, amplitudes, and granulation noise. Astron Astrophys 464: 1059–1067

    Article  ADS  Google Scholar 

  • Leckrone DS (1973). Ultraviolet photometry from the orbiting astronomical observatory. VIII. The blue AP stars. Astrophys J 185: 577–596

    Google Scholar 

  • Ledoux P (1951). The nonradial oscillations of gaseous stars and the problem of beta Canis Majoris. Astrophys J 114: 373–384

    Article  ADS  Google Scholar 

  • Lefèvre L, Marchenko SV, Moffat AFJ, Chené AN, Smith SR, St-Louis N, Matthews JM, Kuschnig R, Guenther DB, Poteet CA, Rucinski SM, Sasselov D, Walker GAH and Weiss WW (2005). Oscillations in the Massive Wolf-Rayet Star WR 123 with the MOST Satellite. Astrophys J 634: L109–L112

    Article  ADS  Google Scholar 

  • Leighton RB, Noyes RW and Simon GW (1962). Velocity Fields in the Solar Atmosphere. I. Preliminary Report. Astrophys J 135: 477–499

    Article  ADS  Google Scholar 

  • Leinert C, Graser U, Waters LBFM, Perrin GS, Jaffe W, Lopez B, Przygodda F, Chesneau O, Schuller PA, Glazenborg-Kluttig AW, Laun W, Ligori S, Meisner JA, Wagner K, Bakker EJ, Cotton B, de Jong J, Mathar R, Neumann U, Storz C (2003) Ten-micron instrument MIDI: getting ready for observations on the VLTI. In: Traub WA (ed) Interferometry for optical astronomy II, Proc. SPIE 4838, pp 893–904

  • Léna PJ, Quirrenbach A (eds) (2000) Interferometry in optical astronomy. Proc. SPIE 4006, 2 parts, 1152 pages. ISBN 0-8194-3631-3

  • Libbrecht KG (1992). On the ultimate accuracy of solar oscillation frequency measurements. Astrophys J 387: 712–714

    Article  ADS  Google Scholar 

  • Lighthill MJ (1952). On sound generated aerodynamically I. General theory. Proc Ry Soc London A211: 564–587

    ADS  MathSciNet  Google Scholar 

  • Lignières F, Rieutord M and Reese D (2006). Acoustic oscillations in rapidly rotating polytropic stars. I. Effects of the centrifugal distortion. Astron Astrophys 455: 607–620

    Article  ADS  Google Scholar 

  • Lochard J, Samadi R and Goupil MJ (2005). Rotation profile inversion in solar-like stars. Astron Astrophys 438: 939–948

    Article  ADS  Google Scholar 

  • Lopez B, Wolf S, Lagarde S, Abraham P, Antonelli P, Augereau JC, Beckman U, Behrend J, Berruyer N, Bresson Y, Chesneau O, Clausse JM, Connot C, Demyk K, Danchi WC, Dugué M, Flament S, Glazenborg A, Graser U, Henning T, Hofmann KH, Heininger M, Hugues Y, Jaffe W, Jankov S, Kraus S, Laun W, Leinert, Ch., Linz H, Mathias, Ph., Meisenheimer K, Matter A, Menut JL, Millour F, Neumann U, Nussbaum E, Niedzielski A, Mosonic L, Petrov R, Ratzka T, Robbe-Dubois S, Roussel A, Schertl D, Schmider FX, Stecklum B, Thiebaut E, Vakili F, Wagner K, Waters LBFM, Weigelt G (2006) MATISSE: perspective of imaging in the mid-infrared at the VLTI. In: Monnier JD, Schöller M, Danchi WC (eds) Advances in stellar interferometry, Proc. SPIE vol 6268, p 62680Z

  • MacGregor KB, Jackson S, Skumanich A and Metcalfe TS (2007). Astrophys J 663: 560–572

    Article  ADS  Google Scholar 

  • Malbet F, Kern PY, Berger JP, Jocou L, Garcia P, Buscher D, Rousselet-Perraut K, Weigelt G, Gai M, Surdej J, Hron J, Neuhäuser R, Le Coarer E, Labeye PR, Le Bouquin J, Benisty M, Herwats E (2006) VSI: a milli-arcsec spectro-imager for the VLTI. In: Monnier JD, Schöller M, Danchi WC (eds) Advances in stellar interferometry, Proc. SPIE, vol 6268, p 62680Y

  • Malbet F, Petrov R, Weigelt G, Chesneau O, Domicianode Souza A, Meilland A, Millour F, Tatulli E and The Amber Consortium (2007). First AMBER/VLTI science. Messenger 127: 37–40

    ADS  Google Scholar 

  • Mantegazza L (2000) Mode detection from line–profile variations. In: Breger M, Montgomery M (eds) Delta Scuti and related stars, ASP Conference Series, vol. 210, pp 138–169

  • Marengo M, Sasselov D, Karovska M, Papaliolios C and Armstrong JT (2002). Theoretical limb darkening for pulsating Cepheids. Astrophys J 567: 1131–1139

    Article  ADS  Google Scholar 

  • Mariotti JM and Ridgway ST (1988). Double Fourier spatio-spectral interferometry – combining high spectral and high spatial resolution in the near infrared. Astron Astrophys 195: 350–363

    ADS  Google Scholar 

  • Marti´c M, Lebrun JC, Appourchaux T and Korzennik SG (2004). p-mode frequencies in solar-like stars: I. Procyon A. Astron Astrophys 418: 295–303

    Article  ADS  Google Scholar 

  • Matthews J (2005) A suitcase full of astrophysics: The MOST microsat and opportunities for low-cost space astronomy. In: Kenneth Seidelmann P, Monet AKB (eds) Astrometry in the age of the next generation of large telescopes, ASP Conference Series, vol 338, p 297

  • Matthews JM, Kurtz DW and Martinez P (1999). Parallaxes versus p-modes: Comparing HIPPARCOS and asteroseismic results for pulsating AP stars. Astrophys J 511: 422–428

    Article  ADS  Google Scholar 

  • Mazumdar A (2005). Asteroseismic diagrams for solar-type stars. Astron Astrophys 441: 1079–1086

    Article  ADS  Google Scholar 

  • Mazumdar A, Briquet M, Desmet M and Aerts C (2006). An asteroseismic study of the β Cephei star β Canis Majoris. Astron Astrophys 459: 589–596

    Article  ADS  Google Scholar 

  • McAlister HA (1976). Spectroscopic binaries as a source for astrometric and speckle interferometric studies. Publ Astron Soc Pacific 88: 317–322

    Article  ADS  Google Scholar 

  • McAlister HA (2000). Why Build Stellar Interferometers?. In: Lawson, PR (eds) Principles of long baseline stellar interferometry, pp 3–8. NASA, JPL, CIT, Pasadena

    Google Scholar 

  • McAlister HA, ten Brummelaar TA, Gies DR, Huang W, Bagnuolo WG, Shure MA, Sturmann J, Sturmann L, Turner NH, Taylor SF, Berger DH, Baines EK, Grundstrom E, Ogden C, Ridgway ST and van Belle G (2005). First results from the CHARA Array. I. An interferometric and spectroscopic study of the fast rotator α Leonis (Regulus). Astrophys J 628: 439–452

    Article  ADS  Google Scholar 

  • Mékarnia D and Gay J (1990). Infrared multispectral interferometry. Astron Astrophys 238: 469–474

    ADS  Google Scholar 

  • Mérand A, Kervella P, Coudé Du Foresto V, Ridgway ST, Aufdenberg JP, ten Brummelaar TA, Berger DH, Sturmann J, Sturmann L, Turner NH and McAlister HA (2005). The projection factor of δ Cephei. A calibration of the Baade-Wesselink method using the CHARA Array. Astron Astrophys 438: L9–L12

    Article  ADS  Google Scholar 

  • Metcalfe TS (2005). Lessons for asteroseismology from white dwarf stars. J Astrophys Astr 26: 273–281

    Article  ADS  Google Scholar 

  • Metcalfe TS and Charbonneau P (2003). Stellar structure modeling using a parallel genetic algorithm for objective global optimization. J Comp Phys 185: 176–193

    Article  MATH  ADS  Google Scholar 

  • Metcalfe TS, Nather RE and Winget DE (2000). Genetic-algorithm-based asteroseismological analysis of the DBV white dwarf GD 358. Astrophys J 545: 974–981

    Article  ADS  Google Scholar 

  • Michel E (2006). Theoretical aspects of asteroseismology. Comm Asteroseismol 147: 40–47

    Article  ADS  Google Scholar 

  • Michelson AA and Pease FG (1921). Measurement of the diameter of alpha Orionis with the interferometer. Astrophys J 53: 249–259

    Article  ADS  Google Scholar 

  • Mieremet al, Braat J, Bokhove H, Ravel K (2000) Achromatic phase shifting using adjustable dispersive elements. In: Léna PJ, Quirrenbach A (eds) Interferometry in optical astronomy, Proc. SPIE, vol 4006, pp 1035–1041

  • Miglio A. and Montalbán J (2005). Constraining fundamental stellar parameters using seismology. Application to α Centauri AB. Astron Astrophys 441: 615–629

    Article  ADS  Google Scholar 

  • Miglio A, Christensen-Dalsgaard J, Di Mauro MP, Monteiro MJPFG and Thompson MJ (2003). Seismic analysis of the helium ionization zones in low- and moderate-mass stars. In: Thompson, MJ, Cunha, MS, and Monteiro, MJPFG (eds) Asteroseismology across the HR diagram, pp 537–540. Kluwer, Dordrecht

    Google Scholar 

  • Miglio A, Montalbán J and Dupret MA (2007a). Instability strips of slowly pulsating B stars and β Cephei stars: the effect of the updated OP opacities and of the metal mixture. Mon Not R Astr Soc 375: L21–L25

    Article  ADS  Google Scholar 

  • Miglio A, Montalbán J and Maceroni C (2007b). 12 Bootis: a test bed for extra-mixing processes in stars. Mon Not R Astr Soc 377: 373–382

    Article  ADS  Google Scholar 

  • Monnier JD (2003). Optical interferometry in astronomy. Rep Prog Phys 66: 789–857

    Article  ADS  Google Scholar 

  • Monnier JD, Schöller M, Danchi WC (2006) Advances in stellar interferometry. Proc. SPIE, vol 6268, ISBN 9780819463333

  • Monnier JD, Zhao M, Pedretti E, Thureau N, Ireland M, Muirhead P, Berger JP, Millan-Gabet R, Van Belle G, ten Brummelaar T, McAlister H, Ridgway S, Turner N, Sturmann L, Sturmann J and Berger D (2007). Imaging the Surface of Altair. Science 317: 342–345

    Article  ADS  Google Scholar 

  • Monteiro MJPFG and Thompson MJ (1998). On the seismic signature of the HeII ionization zone in stellar envelopes. In: Deubner, FL, Christensen-Dalsgaard, J and Kurtz, DW (eds) Proc. IAU Symp. 185: New eyes to see inside the Sun and stars, pp 317–318. Kluwer, Dordrecht

    Google Scholar 

  • Monteiro MJPFG and Thompson MJ (2005). Seismic analysis of the second ionization region of helium in the Sun—I. Sensitivity study and methodology. Mon Not R Astr Soc 361: 1187–1196

    Article  ADS  Google Scholar 

  • Monteiro MJPFG, Christensen-Dalsgaard J and Thompson MJ (1996). Seismic properties of the Sun’s superadiabatic layer I. Theoretical modelling and parametrisation of the uncertainties. Astron Astrophys 306: 624–634

    ADS  Google Scholar 

  • Monteiro MJPFG, Christensen-Dalsgaard J and Thompson MJ (2000). Seismic study of stellar convective regions: the base of the convective envelope in low-mass stars. Mon Not R Astr Soc 316: 165–172

    Article  ADS  Google Scholar 

  • Monteiro MJPFG, Christensen-Dalsgaard J, Thompson MJ (2002) Asteroseismic Inference for Solar-Type Stars. In: Favata F, Roxburgh IW, Galadí-Enríquez D (eds) Proc. 1st Eddington workshop, ‘stellar structure and habitable planet finding’, ESA SP-485, ESA Publications Division, Noordwijk, pp 291–298

  • Montgomery MH (2005). A new technique for probing convection in pulsating white dwarf stars. Astrophys J 633: 1142–1149

    Article  ADS  Google Scholar 

  • Montgomery MH and O’Donoghue DO (1999). A derivation of the errors for least squares fitting to time series data. Delta Scuti Newslett 13: 28

    ADS  Google Scholar 

  • Montgomery MH, Metcalfe TS and Winget DE (2003). The core/envelope symmetry in pulsating stars. Mon Not R Astr Soc 344: 657–664

    Article  ADS  Google Scholar 

  • Mozurkewich D, Johnston KJ, Simon RS, Bowers PF, Gaume R, Hutter DJ, Colavita MM, Shao M and Pan XP (1991). Angular diameter measurements of stars. Astron J 101: 2207–2219

    Article  ADS  Google Scholar 

  • Mozurkewich D, Armstrong JT, Hindsley RB, Quirrenbach A, Hummel CA, Hutter DJ, Johnston KJ, Elias NM, Hajian AR, Buscher DF and Simon RS (2003). Angular diameters of stars from the Mark III optical interferometer. Astron J 126: 2502–2520

    Article  ADS  Google Scholar 

  • Mosser B (2006) SIAMOIS: an asteroseismic network with 1 site. in Antarctica. In: Fletcher K (ed) Proc. SOHO 18 / GONG 2006 HELAS I Conference beyond the spherical Sun, ESA SP-624, ESA Publications Division, Noordwijk

  • Mourard D, Abe L, Domiciano A, Bonneau D, Blazit A, Vakili F, Stee P (2003) Status report on the GI2T interferometer. In: Traub WA (eds) Interferometry for optical astronomy II, Proc. SPIE, vol 4838, pp 9–18

  • Moya A, Suárez JC, Amado PJ, Martin-Ruíz S and Garrido R (2005). Frequency ratio method for seismic modeling of γ Doradus stars. Astron Astrophys 432: 189–198

    Article  ADS  Google Scholar 

  • Munteanu A, Bono G, José J, García-Berro E and Stellingwerf RF (2005). Limit-cycle behaviour in one-zone convective models. Astrophys J 627: 454–463

    Article  ADS  Google Scholar 

  • Muterspaugh MW, Lane BF, Konacki M, Burke BF, Colavita MM, Kulkarni SR and Shao M (2005). PHASES high-precision differential astrometry of δ Equulei. Astron J 130: 2866–2875

    Article  ADS  Google Scholar 

  • Muterspaugh MW, Lane BF, Konacki M, Wiktorowicz S, Burke BF, Colavita MM, Kulkarni SR and Shao M (2006). PHASES differential astrometry and iodine cell radial velocities of the κ Pegasi triple star system. Astrophys J 636: 1020–1032

    Article  ADS  Google Scholar 

  • Nordlund Å (1982). Numerical simulations of the solar granulation. I - Basic equations and methods. Astron Astrophys 107: 1–10

    MATH  ADS  Google Scholar 

  • Nordlund Å and Stein RF (1991). Granulation: non-adiabatic patterns and shocks. In: Gough, DO and Toomre, J (eds) Challenges to theories of the structure of moderate-mass stars, Lecture notes in physics, vol 388, pp 141–146. Springer, Heidelberg

    Google Scholar 

  • North JR, Davis J, Bedding TR, Ireland MJ, Jacob AP, O’Byrne J, Owens SM, Robertson JG, Tango WJ and Tuthill PG (2007a). The radius and mass of the subgiant star β Hyi from interferometry and asteroseismology. Mon Not R Astr Soc 380: L80–L83

    Article  ADS  Google Scholar 

  • North JR, Davis J, Tuthill PG, Tango WJ and Robertson JG (2007b). Orbital solution & fundamental parameters of σ Scorpii. Mon Not Ry Astr Soc 380: 1276–1284

    Article  ADS  Google Scholar 

  • North JR, Tuthill PG, Tango WJ and Davis J (2007c). γ2 Velorum: orbital solution and fundamental parameter determination with SUSI. Mon Not Ry Astr Soc 377: 415–424

    Article  ADS  Google Scholar 

  • Nowakowski RM (2005). Multimode resonant coupling in pulsating stars. Acta Astron 55: 1–41

    ADS  Google Scholar 

  • Ohishi N, Nordgren TE and Hutter DJ (2004). Asymmetric surface brightness distribution of Altair observed with the navy prototype optical interferometer. Astrophys J 612: 463–471

    Article  ADS  Google Scholar 

  • Ohnaka K, Bergeat J, Driebe T, Graser U, Hofmann KH, Köhler R, Leinert C, Lopez B, Malbet F, Morel S, Paresce F, Perrin G, Preibisch T, Richichi A, Schertl D, Schöller M, Sol H, Weigelt G and Wittkowski M (2005). Mid-infrared interferometry of the Mira variable RR Sco with the VLTI MIDI instrument. Astron Astrophys 429: 1057–1067

    Article  ADS  Google Scholar 

  • Olivier EA and Wood PR (2005). Non-linear pulsation models of red giants. Mon Not R Astr Soc 362: 1396–1412

    Article  ADS  Google Scholar 

  • Ollivier M (2006). PEGASE: a DARWIN/TPF pathfinder. In: Aime, C and Vakili, F (eds) Direct imaging of exoplanets: science and techniques, IAU Colloquium 200, pp 241. Cambridge University Press, Cambridge

    Google Scholar 

  • Osaki Y (1975). Nonradial oscillations of a 10 solar mass star in the main-sequence stage. Publ Astron Soc Japan 27: 237–258

    ADS  Google Scholar 

  • Otí Floranes H, Christensen-Dalsgaard J and Thompson MJ (2005). The use of frequency-separation ratios for asteroseismology. Mon Not R Astr Soc 356: 671–679

    Article  ADS  Google Scholar 

  • Pamyatnykh AA (1999). Pulsational instability domains in the upper main sequence. Acta Astron 49: 119–148

    ADS  Google Scholar 

  • Pamyatnykh AA, Handler G and Dziembowski WA (2004). Asteroseismology of the β Cephei star ν Eridani: interpretation and applications of the oscillation spectrum. Mon Not R Astr Soc 350: 1022–1028

    Article  ADS  Google Scholar 

  • Pan XP, Shao M, Colavita MM, Mozurkewich D, Simon RS and Johnston KJ (1990). Apparent orbit of the spectroscopic binary  beta Arietis with the Mark III stellar interferometer. Astrophys J 356: 641–645

    Article  ADS  Google Scholar 

  • Pan XP, Shao M, Colavita MM, Armstrong JT, Mozurkewich D, Vivekanand M, Denison CS, Simon RS and Johnston KJ (1992). Determination of the visual orbit of the spectroscopic binary α Andromedae with submilliarcsecond precision. Astrophys J 384: 624–633

    Article  ADS  Google Scholar 

  • Paresce F (1997) Science with the VLT Interferometer. Springer-verlag, series: ESO astrophysics symposia, ISBN 3540632646

  • Pasquini L, Alonso J, Avila G, Barriga P, Biereichel P, Buzzoni B, Cavadore C, Cumani C, Dekker H, Delabre B, Kaufer A, Kotzlowski H, Hill V, Lizon JL, Nees W, Santin P, Schmutzer R, Kesteren AV, Zoccali M (2003) Installation and first results of FLAMES, the VLT multifibre facility. In: Iye M, Moorwood AFM (eds) Instrument design and performance for optical/infrared groundbased telescopes, Proc. SPIE, vol 4841, pp 1682–1693

  • Paternò L, Ventura R, Canuto VM and Mazzitelli I (1993). Helioseismological test of a new model for stellar convection. Astrophys J 402: 733–740

    Article  ADS  Google Scholar 

  • Pérez Hernández F and Christensen-Dalsgaard J (1998). The phase function for stellar acoustic oscillations - IV. Solar-like stars. Mon Not R Ast Soc 295: 344–352

    Article  ADS  Google Scholar 

  • Perrin G (2003). The calibration of interferometric visibilities obtained with single-mode optical interferometers. Computation of error bars and correlations. Astron Astrophys 400: 1173–1181

    ADS  Google Scholar 

  • Perrin G and Ridgway ST (2005). Squared Visibility Estimators: Calibrating Biases to Reach Very High Dynamic Range. Astrophys J 626: 1138–1148

    Article  ADS  Google Scholar 

  • Perrin G, Ridgway ST, Coudédu Foresto V, Mennesson B, Traub WA and Lacasse MG (2004). Interferometric observations of the supergiant stars α Orionis and α Herculis with FLUOR at IOTA. Astron Astrophys 418: 675–685

    Article  ADS  Google Scholar 

  • Perrin G, Woillez J, Lai O, Guérin J, Kotani T, Wizinowich PL, Le Mignant D, Hrynevych M, Gathright J, Léna P, Chaffee F, Vergnole S, Delage L, Reynaud F, Adamson AJ, Berthod C, Brient B, Collin C, Crétenet J, Dauny F, Deléglise C, Fédou P, Goeltzenlichter T, Guyon O, Hulin R, Marlot C, Marteaud M, Melse BT, Nishikawa J, Reess JM, Ridgway ST, Rigaut F, Roth K, Tokunaga AT and Ziegler D (2006). Interferometric coupling of the Keck telescopes with single-mode fibers. Science 311: 194

    Article  ADS  Google Scholar 

  • Perryman MAC, Lindegren L, Kovalevsky J, Hoeg E, Bastian U, Bernacca PL, Crézé M, Donati F, Grenon M, van Leeuwen F, van der Marel H, Mignard F, Murray CA, Le Poole RS, Schrijver H, Turon C, Arenou F, Froeschlé M and Petersen CS (1997). The Hipparcos Catalogue. Astron Astrophys 323: L49–L52

    ADS  Google Scholar 

  • Pesnell WD (1987). A new driving mechanism for stellar pulsations. Astrophys J 314: 598–604

    Article  ADS  Google Scholar 

  • Peterson DM, Hummel CA, Pauls TA, Armstrong JT, Benson JA, Gilbreath GC, Hindsley RB, Hutter DJ, Johnston KJ, Mozurkewich D and Schmitt HR (2006c). Vega is a rapidly rotating star. Nature 440: 896–899

    Article  ADS  Google Scholar 

  • Peterson DM, Hummel CA, Pauls TA, Armstrong JT, Benson JA, Gilbreath GC, Hindsley RB, Hutter DJ, Johnston KJ, Mozurkewich D and Schmitt H (2006b). Resolving the effects of rotation in Altair with long-baseline interferometry. Astrophys J 636: 1087–1097

    Article  ADS  Google Scholar 

  • Petrov RG (1989) Differential interferometry. In: Alloin DM, Mariotti JM (eds) Diffraction-limited imaging with very large telescopes, NATO ASI vol 274, pp 249–271

  • Petrov RG & Amber Consortium, The (2003) The near infrared VLTI instrument AMBER. In: Perrin G, Malbet F (eds) Observing with the VLTI, EAS Publications Series vol 6, pp 111–126

  • Petrov RG, Malbet F, Weigelt G, Antonelli P, Beckmann U, Bresson Y, Chelli A, Dugué M, Duvert G, Gennari S, Glück L, Kern P, Lagarde S, Le Coarer E, Lisi F, Millour F, Perraut K, Puget P, Rantakyrö F, Robbe-Dubois S, Roussel A, Salinari P, Tatulli E, Zins G, Accardo M, Acke B, Agabi K, Altariba E, Arezki B, Aristidi E, Baffa C, Behrend J, Blöcker T, Bonhomme S, Busoni S, Cassaing F, Clausse JM, Colin J, Connot C, Delboulbé A, Domicianode Souza A, Driebe T, Feautrier P, Ferruzzi D, Forveille T, Fossat E, Foy R, Fraix-Burnet D, Gallardo A, Giani E, Gil C, Glentzlin A, Heiden M, Heininger M, Hernandez Utrera O, Hofmann KH, Kamm D, Kiekebusch M, Kraus S, Le Contel D, Le Contel JM, Lesourd T, Lopez B, Lopez M, Magnard Y, Marconi A, Mars G, Martinot-Lagarde G, Mathias P, Mège P, Monin JL, Mouillet D, Mourard D, Nussbaum E, Ohnaka K, Pacheco J, Perrier C, Rabbia Y, Rebattu S, Reynaud F, Richichi A, Robini A, Sacchettini M, Schertl D, Schöller M, Solscheid W, Spang A, Stee P, Stefanini P, Tallon M, Tallon-Bosc I, Tasso D, Testi L, Vakili F, von der Lühe O, Valtier JC, Vannier M and Ventura N (2007). AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument. Astron Astrophys 464: 1–12

    Article  ADS  Google Scholar 

  • Pickering EC (1912) Periods of 25 variable stars in the smal magellanic cloud. Harvard College Observatory, circular 173, Harvard

  • Pigulski A (2006) Intrinsic variability in multiple systems and clusters: an overview. In: Sterken C Aerts C (eds) Astrophysics of variable stars, ASP Conference Series, vol 349, p 137

  • Pijpers FP (2006) Methods in helio- and asteroseismology. Imperial College Press

  • Pijpers FP and Thompson MJ (1992). Faster formulations of the optimally localized averages method for helioseismic inversion. Astron Astrophys 262: L33–L36

    ADS  Google Scholar 

  • Pijpers FP and Thompson MJ (1994). The SOLA method for helioseismic inversion. Astron Astrophys 281: 231–240

    ADS  Google Scholar 

  • Pijpers FP, Teixeira TC, Garcia PJ, Cunha MS, Monteiro MJPFG and Christensen-Dalsgaard J (2003). Interferometry and asteroseismology: The radius of τ Cet. Astron Astrophys 406: L15–L18

    Article  ADS  Google Scholar 

  • Poretti E, Buzasi D, Laher R, Catanzarite J and Conrow T (2002). Asteroseismology from space: The delta Scuti star theta 2 Tauri monitored by the WIRE satellite. Astron Astrophys 382: 157–163

    Article  ADS  Google Scholar 

  • Pourbaix D, Nidever D, McCarthy C, Butler RP, Tinney CG, Marcy GW, Jones HRA, Penny AJ, Carter BD, Bouchy F, Pepe F, Hearnshaw JB, Skuljan J, Ramm D and Kent D (2002). Constraining the difference in convective blueshift between the components of α Centauri with precise radial velocities. Astron Astrophys 386: 280–285

    Article  ADS  Google Scholar 

  • Pourbaix D, Tokovinin AA, Batten AH, Fekel FC, Hartkopf WI, Levato H, Morrell NI, Torres G and Udry S (2004). SB9: the ninth catalogue of spectroscopic binary orbits. Astron Astrophys 424: 727–732

    Article  ADS  Google Scholar 

  • Press WH, Flannery BP, Teukolsky SA, Vetterling WT (1986) Numerical Recipes, Cambridge, Sect 5

  • Provost J and Berthomieu G (1986). Asymptotic properties of low degree solar gravity modes. Astron Astrophys 165: 218–226

    MATH  ADS  Google Scholar 

  • Quirrenbach A (2000) Principles of long baseline stellar interferometry. In: Lawson PR (ed) Course notes from the 1999 Michelson Summer School, held August 15–19, 1999, National Aeronautics and Space Administration, Jet Propulsion Laboratory, Passadena, p 71

  • Quirrenbach A (2001a). Optical Interferometry. Annu Rev Astron Astrophys 39: 353–401

    Article  ADS  Google Scholar 

  • Quirrenbach A (2001b) Optical and infrared long-baseline interferometry: application to binary star science. In: Zinnecker H, Mathieu RD (eds) Proc. IAU Symposium 200, the formation of binary stars, pp 539–546

  • Quirrenbach A (2004a) Interferometric high-resolution spectroscopy. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. SPIE, vol 5491, pp 146–153

  • Quirrenbach A (2004b) Design considerations for an Extremely Large Synthesis Array. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. SPIE, vol 5491, pp 1563–1573

  • Quirrenbach A, Aufdenberg J (2004) Wavelength-dependent diameters of cool giant stars. In: Piskunov N, Weiss WW, Gray DF (eds) Modelling of stellar atmospheres, IAU Symposium 210, E68

  • Quirrenbach A, Mozurkewich D, Armstrong JT, Johnston KJ, Colavita MM and Shao M (1992). Interferometric observations of Mira (o Ceti). Astron Astrophys 259: L19–L22

    ADS  Google Scholar 

  • Quirrenbach A, Mozurkewich D, Armstrong JT, Buscher DF and Hummel CA (1993). Angular diameter measurements of cool giant stars in strong TiO bands and in the continuum. Astrophys J 406: 215–219

    Article  ADS  Google Scholar 

  • Quirrenbach A, Mozurkewich D, Buscher DF, Hummel CA and Armstrong JT (1996). Angular diameter and limb darkening of Arcturus. Astron Astrophys 312: 160–166

    ADS  Google Scholar 

  • Quirrenbach A, Bjorkman KS, Bjorkman JE, Hummel CA, Buscher DF, Armstrong JT, Mozurkewich D, Elias NM and Babler BL (1997). Constraints on the geometry of circumstellar envelopes: Optical interferometric and spectropolarimetric observations of seven Be stars. Astroph J 479: 477–496

    Article  ADS  Google Scholar 

  • Quirrenbach A, Coudé du Foresto V, Daigne G, Hofmann KH, Hofmann R, Lattanzi M, Osterbart R, le Poole R, Queloz D, Vakili F (1998) PRIMA—study for a dual-beam instrument for the VLT Interferometer. In: Reasenberg RD (ed) Astronomical interferometry, Proc. of the SPIE 3350, pp 807–817

  • Quirrenbach A, Henning T, Queloz D, Albrecht S, Bakker E, Baumeister H, Bizenberger P, Bleuler H, Dändliker R, de Jong J, Fleury M, Frink S, Gillet D, Jaffe W, Hanenburg SH, Hekker S, Launhardt R, le Poole R, Maire C, Mathar R, Mullhaupt P, Murakawa K, Pepe F, Pragt J, Sache L, Scherler O, Ségransan D, Setiawan J, Sosnowska D, Tubbs R, Venema L, Wagner K, Weber L, Wüthrich R (2004) The PRIMA astrometric planet search project. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. SPIE, vol 5491, pp 424–432

  • Rabello-Soares MC, Basu S and Christensen-Dalsgaard J (1999). On the choice of parameters in solar structure inversion. Mon Not R Astr Soc 309: 35–47

    Article  ADS  Google Scholar 

  • Ragland S, Traub WA, Berger JP, Danchi WC, Monnier JD, Willson LA, Carleton NP, Lacasse MG, Millan-Gabet R, Pedretti E, Schloerb FP, Cotton WD, Townes CH, Brewer M, Haguenauer P, Kern P, Labeye P, Malbet F, Malin D, Pearlman M, Perraut K, Souccar K and Wallace G (2006). First surface-resolved results with the infrared optical telescope array imaging interferometer: detection of asymmetries in asymptotic giant branch stars. Astrophys J 652: 650–660

    Article  ADS  Google Scholar 

  • Randall SK, Matthews JM, Fontaine G, Rowe J, Kuschnig R, Green EM, Brassard P, Chayer P, Guenther DB, Moffat AFJ, Rucinski S, Sasselov D, Walker GAH and Weiss WW (2005a). Detection of long-period variations in the subdwarf B star PG 0101+039 on the basis of photometry from the MOST satellite. Astrophys J 633: 460–464

    Article  ADS  Google Scholar 

  • Randall SK, Fontaine G, Brassard P and Bergeron P (2005b). The potential of multicolor photometry for pulsating subdwarf B stars. Astrophys J Suppl 161: 456–479

    Article  ADS  Google Scholar 

  • Rantakyro FT, Galliano E, Hummel CA, Kaufer A, Kervella P, Morel S, Schöller M, Vannier M, Wittkowski M. (2004) VLTI science operations at Paranal. In: Traub WA (ed) New frontiers in stellar interferometry, Proc. SPIE, vol 5491, p 1690

  • Reese D, Lignières F and Rieutord M (2006a). Oscillations of rapidly rotating stars. Comm Asteroseismol 147: 65–68

    Article  ADS  Google Scholar 

  • Reese D, Lignières F and Rieutord M (2006b). Acoustic oscillations of rapidly rotating polytropic stars. II. Effects of the Coriolis and centrifugal accelerations. Astron Astrophys 455: 621–637

    Article  ADS  Google Scholar 

  • Rice JB (2002). Doppler imaging of stellar surfaces—techniques and issues. Astron Nachrichten 323: 220–235

    Article  ADS  Google Scholar 

  • Ridgway ST, Roddier FJ (2000) Infrared very large array for the 21st century. In: Léna PJ, Quirrenbach A (eds) Interferometry in optical astronomy, Proc. SPIE, vol 4006, pp 940–950

  • Rieutord M (2006a). The dynamics of the radiative envelope of rapidly rotating stars. I. A spherical Boussinesq model. Astron Astrophys 451: 1025–1036

    Article  MATH  ADS  Google Scholar 

  • Rieutord M (2006b) Modeling rapidly rotating stars. In: Barret D, Casoli F, Lagache G, Lecavelier A, Pagani L (eds) Proceedings of the annual meeting of the French Society of Astronomy and Astrophysics, p 501

  • Rivinius TH, Baade D and Stefl S (2003). Non-radially pulsating Be stars. Astron Astrophys 411: 229–247

    Article  ADS  Google Scholar 

  • Robe H (1968). Les oscillations non radiales des polytropes. Ann d’Astrophys 31: 475–482

    ADS  Google Scholar 

  • Robinson FJ, Demarque P, Li LH, Kim YC, Chan KL and Guenther DB (2003). Three-dimensional convection simulations of the outer layers of the Sun using realistic physics. Mon Not R Astr Soc 340: 923–936

    Article  ADS  Google Scholar 

  • Roca Cortés T, Montańés P, Pallé PL, Pérez Hernández F, Jiménez A, Régulo C, and the GOLF Team (1999) Low â„“ solar p-mode oscillation parameters and convection. In: Giménez A, Guinan EF, Montesinos B (eds) Theory and tests of convection in stellar structure, ASP Conference Series, vol 173, pp 305–308

  • Rodríguez E and Breger M (2001). δ Scuti and related stars: analysis of the R00 Catalogue. Astron Astrophys 366: 178–196

    Article  ADS  Google Scholar 

  • Rosenthal CS, Christensen-Dalsgaard J, Nordlund Å, Stein RF and Trampedach R (1999). Convective contributions to the frequencies of solar oscillations. Astron Astrophys 351: 689–700

    ADS  Google Scholar 

  • Roxburgh IW (2004). 2-Dimensional models of rapidly rotating stars. I. Uniformly rotating zero age main sequence stars. Astron Astrophys 428: 171–179

    Article  MATH  ADS  Google Scholar 

  • Roxburgh IW (2005). The ratio of small to large separations of stellar p-modes. Astron Astrophys 434: 665–669

    Article  ADS  Google Scholar 

  • Roxburgh IW (2006). 2-Dimensional models of rapidly rotating stars. II. Hydrostatic and acoustic models with Ω  =  Ω(r,θ). Astron Astrophys 454: 883–888

    Article  ADS  Google Scholar 

  • Roxburgh IW and Vorontsov SV (1994). The seismology of stellar cores: a simple theoretical description of the ‘small frequency separations’. Mon Not R Astr Soc 267: 297–302

    ADS  Google Scholar 

  • Roxburgh IW and Vorontsov SV (2000). Semiclassical approximation for low-degree stellar p modes – II. Classical ray tracing. Mon Not R ast Soc 317: 151–157

    ADS  Google Scholar 

  • Roxburgh IW and Vorontsov SV (2001). Semiclassical approximation for low-degree stellar p modes – III. Acoustic resonances and diagnostic properties of the oscillation frequencies. Mon Not R ast Soc 322: 85–96

    Google Scholar 

  • Roxburgh IW and Vorontsov SV (2003). The ratio of small to large separations of acoustic oscillations as a diagnostic of the interior of solar-like stars. Astron Astrophys 411: 215–220

    Article  ADS  Google Scholar 

  • Roxburgh IW and Vorontsov SV (2006). The autocorrelation function of stellar p-mode measurements and its diagnostic properties. Mon Not R Astr Soc 369: 1491–1496

    Article  ADS  Google Scholar 

  • Ryabchikova TA, Landstreet JD, Gelbmann MJ, Bolgova GT, Tsymbal VV and Weiss WW (1997). Abundance analysis of roAp stars. IV. HD24712. Astron Astrophys 327: 1137–1146

    ADS  Google Scholar 

  • Sabbey CN, Sasselov DD, Fieldus MS, Lester JB, Venn KA and Butler RP (1995). On spectral line formation and measurement in Cepheids: implications to distance determination. Astrophys J 446: 250–260

    Article  ADS  Google Scholar 

  • Saio H (1981). Rotational and tidal perturbations of nonradial oscillations in a polytropic star. Astrophys J 244: 299–315

    Article  ADS  Google Scholar 

  • Saio H (2005). A non-adiabatic analysis for axisymmetric pulsations of magnetic stars. Mon Not R Astr Soc 360: 1022–1032

    Article  ADS  Google Scholar 

  • Saio H and Gautschy A (2004). Axisymmetric p-mode pulsations of stars with dipole magnetic fields. Mon Not R Astr Soc 350: 485–505

    Article  ADS  Google Scholar 

  • Saio H, Kuschnig R, Gautschy A, Cameron C, Walker GAH, Matthews JM, Guenther DB, Moffat AFJ, Rucinski SM, Sasselov D and Weiss WW (2006). MOST Detects g- and p-modes in the B supergiant HD 163899 (B2 Ib/II). Astrophys J 650: 1111–1118

    Article  ADS  Google Scholar 

  • Saio H, Cameron C, Kuschnig R, Walker GAH, Matthews JM, Rowe JF, Lee U, Huber D, Weiss WW, Guenther DB, Moffat AFJ, Rucinski SM and Sasselov D (2007). MOST Detects g-Modes in the Late-Type Be Star β Canis Minoris (B8 Ve). Astrophys J 654: 544–550

    Article  ADS  Google Scholar 

  • Samadi R, Nordlund Å, Stein RF, Goupil MJ and Roxburgh I (2003a). Numerical 3D constraints on convective eddy time-correlations: consequences for stochastic excitation of solar p modes. Astron Astrophys 404: 1129–1137

    Article  ADS  Google Scholar 

  • Samadi R, Nordlund Å, Stein RF, Goupil MJ and Roxburgh I (2003b). Numerical constraints on the model of stochastic excitation of solar-type stars. Astron Astrophys 403: 303–312

    Article  ADS  Google Scholar 

  • Samadi R, Goupil MJ, Alecian E, Baudin F, Georgobiani D, Trampedach R, Stein R and Nordlund Å (2005). Excitation of solar-like oscillations: from PMS to MS stellar models. J Astrophys Astr 26: 171–184

    Article  ADS  Google Scholar 

  • Samadi R, Kupka F, Goupil MJ, Lebreton Y and van’t Veer-Menneret C (2006). Influence of local treatments of convection upon solar p mode excitation rates. Astron Astrophys 445: 233–242

    Article  ADS  Google Scholar 

  • Scargle JD (1982). Studies in astronomical time series analysis. II—Statistical aspects of spectral analysis of unevenly spaced data. Astrophys J 263: 835–853

    Article  ADS  Google Scholar 

  • Scherrer PH, Wilcox JM, Christensen-Dalsgaard J and Gough DO (1983). Detection of solar five-minute oscillations of low degree. Solar Phys 82: 75–87

    Article  ADS  Google Scholar 

  • Schmitz F and Fleck B (1998). On wave equations and cut-off frequencies of plane atmospheres. Astron Astrophys 337: 487–494

    ADS  Google Scholar 

  • Schou J, Buzasi DL (2001) Observations of p-modes in α Cen. In: Wilson A (ed) SOHO 10/GONG 2000 workshop: helio- and asteroseismology at the dawn of the millennium. ESA SP-464, pp 391–394

  • Schou J, Antia HM, Basu S, Bogart RS, Bush RI, Chitre SM, Christensen-Dalsgaard J, Di Mauro MP, Dziembowski WA, Eff-Darwich A, Gough DO, Haber DA, Hoeksema JT, Howe R, Korzennik SG, Kosovichev AG, Larsen RM, Pijpers FP, Scherrer PH, Sekii T, Tarbell TD, Title AM, Thompson MJ and Toomre J (1998). Helioseismic studies of differential rotation in the solar envelope by the Solar Oscillations Investigation using the Michelson Doppler Imager. Astrophys J 505: 390–417

    Article  ADS  Google Scholar 

  • Schrijvers C, Telting JH, Aerts C, Ruymaekers E and Henrichs HF (1997). Line-profile variations due to adiabatic non-radial pulsations in rotating stars. I. Observable characteristics of spheroidal modes. Astron Astrophys Suppl 121: 343–368

    Article  ADS  Google Scholar 

  • Schwarzenberg-Czerny A (1997). The Correct Probability Distribution for the Phase Dispersion Minimization Periodogram. Astrophys J 489: 941–945

    Article  ADS  Google Scholar 

  • Scuflaire R (1974). The non radial oscillations of condensed polytropes. Astron Astrophys 36: 107–111

    ADS  Google Scholar 

  • Seaton MJ (2005). Opacity Project data on CD for mean opacities and radiative accelerations. Mon Not R Astr Soc 362: L1–L3

    Article  ADS  Google Scholar 

  • Ségransan D, Kervella P, Forveille T and Queloz D (2003). First radius measurements of very low mass stars with the VLTI. Astron Astrophys 397: L5–L8

    Article  ADS  Google Scholar 

  • Shao M, (ed) (2003) Interferometry in Space. Proc. SPIE, vol 4852, ISBN 9780819446312

  • Shao M and Colavita MM (1992). Long-baseline optical and infrared stellar interferometry. Annu Rev Astron Astrophys 30: 457–498

    Article  ADS  Google Scholar 

  • Shapley H (1914). On the Nature and Cause of Cepheid Variation. Astrophys J 40: 448–465

    Article  ADS  Google Scholar 

  • Shobbrook RR, Handler G, Lorenz D and Mogorosi D (2006). Photometric studies of three multiperiodic β Cephei stars: β CMa, 15 CMa and KZ Mus. Mon Not R Astr Soc 369: 171–181

    Article  ADS  Google Scholar 

  • Smeyers P (1968). Sur la forme asymptotique des modes non radiaux dans les étoiles massives. Ann d’Astrophys 31: 159–165

    ADS  Google Scholar 

  • Smith MA (1985a). The nonradial oscillations of Spica. I - Two commensurable modes. II - A ’quasi-toroidal’ mode. Astrophys J 297: 206–232

    Article  ADS  Google Scholar 

  • Smith MA (1985b). The nonradial oscillations of SPICA—part two—a Quasi-toroidal mode. Astrophys J 297: 224–232

    Article  ADS  Google Scholar 

  • Smolec R and Moskalik P (2007). Amplitude saturation in β Cephei models. Mon Not R Astr Soc 377: 645–656

    Article  ADS  Google Scholar 

  • Soufi F, Goupil MJ and Dziembowski WA (1998). Effects of moderate rotation on stellar pulsation. I. Third order perturbation formalism. Astron Astrophys 334: 911–924

    ADS  Google Scholar 

  • Stamford PA and Watson RD (1981). Baade-Wesselink and related techniques for mode discrimination in nonradial stellar pulsations. Astrophys Space Sci 77: 131–158

    Article  ADS  Google Scholar 

  • Stankov A and Handler G (2005). Catalog of galactic β cephei stars. Astrophys J Suppl 158: 193–216

    Article  ADS  Google Scholar 

  • Stein RF (1968). Waves in the solar atmosphere. I. The acoustic energy flux. Astrophys J 154: 297–306

    Article  ADS  Google Scholar 

  • Stein RF and Nordlund Å (1989). Topology of convection beneath the solar surface. Astrophys J 342: L95–L98

    Article  ADS  Google Scholar 

  • Stein RF and Nordlund Å (1998). Simulations of solar granulation. I. General properties. Astrophys J 499: 914–933

    Article  ADS  Google Scholar 

  • Stein RF and Nordlund Å (2001). Solar oscillations and convection: II. Excitation of radial oscillations. Astrophys J 546: 585–603

    Article  ADS  Google Scholar 

  • Stein R, Georgobiani D, Trampedach R, Ludwig HG and Nordlund Å (2004). Excitation of radial p-modes in the Sun and stars. Solar Phys 220: 229–242

    Article  ADS  Google Scholar 

  • Stein RF, Benson D, Georgobiani D and Nordlund Å (2006). Supergranule scale convection simulations. In: Fletcher, K (eds) Proceedings SOHO 18 / GONG 2006 / HELAS I Conference Beyond the spherical Sun, ESA SP-624, pp 1–4. ESA Publications Division, Noordwijk

    Google Scholar 

  • Stellingwerf RF (1982). Convection in pulsating stars. I. Nonlinear hydrodynamics. Astrophys J 262: 330–338

    Article  ADS  Google Scholar 

  • Stellingwerf RF (1984). Convection in pulsating stars. III. The RR Lyrae instability strip. Astrophys J 277: 322–326

    Article  ADS  Google Scholar 

  • Stello D, Kjeldsen H, Bedding TR and Buzasi D (2006). Oscillation mode lifetimes in ξ Hydrae: will strong mode damping limit asteroseismology of red giant stars. Astron Astrophys 448: 709–715

    Article  ADS  Google Scholar 

  • Suárez JC, Bruntt H and Buzasi D (2005). Modelling of the fast rotating δ Scuti star Altair. Astron Astrophys 438: 633–641

    Article  ADS  Google Scholar 

  • Surdej J, Caro D, Detal A, eds (2005) Science cases for next generation optical/infrared interferometric facilities. In: Proceedings of the 37th Liège international astrophysical colloquium. Liège University, Liège

  • Surdej J, Caro D, Detal A (eds) (2006) Technology roadmap for future inteferometric facilities. Liège University

  • Svensson F and Ludwig HG (2005). Hydrodynamical simulations of convection-related stellar micro-variability. In: Favata, F, Hussain, G and Battrick, B (eds) Proc 13th Cool Stars Workshop, Hamburg, 5–9 July 2004, ESA SP-560, pp 979–984. ESA Publication Division, Noordwijk

    Google Scholar 

  • Söderhjelm S. (1999). Visual binary orbits and masses post Hipparcos. Astron Astrophys 341: 121–140

    ADS  Google Scholar 

  • Takata M (2005). Momentum conservation and model classification of the dipolar oscillations in stars. Publ Astron Soc Jpn 57: 375–389

    ADS  Google Scholar 

  • Tango WJ, Davis J, Ireland MJ, Aerts C, Uytterhoeven K, Jacob AP, Mendez A, North JR, Seneta EB and Tuthill PG (2006). Orbital elements, masses and distance of λ Scorpii A and B determined with the Sydney University Stellar Interferometer and high-resolution spectroscopy. Mon Not R Astr Soc 370: 884–890

    ADS  Google Scholar 

  • Tassoul M (1980). Asymptotic approximations for stellar nonradial pulsations. Astrophys J Suppl 43: 469–490

    Article  ADS  Google Scholar 

  • Tassoul M (1990). Second-order asymptotic approximations for stellar nonradial acoustic modes. Astrophys J 358: 313–327

    Article  ADS  Google Scholar 

  • Telting JH, Aerts C and Mathias P (1997). A period analysis of the optical line variability of β Cephei: evidence for multi-mode pulsation and rotational modulation. Astron Astrophys 322: 493–506

    ADS  Google Scholar 

  • Telting JH and Schrijvers C (1997). Line-profile variations of non-radial adiabatic pulsations of rotating stars. II. The diagnostic value of amplitude and phase diagrams derived from time series of spectra. Astron Astrophys 317: 723–741

    ADS  Google Scholar 

  • Telting JH and Schrijvers C (1998). A new bright beta Cephei star: line–profile variability in omega1 SCO. Astron Astrophys 339: 150–158

    ADS  Google Scholar 

  • Teixeira TC, Emerson JP and Palumbo ME (1998). Ice CO-cktails in molecular cloud cores. Astron Astrophys 330: 711–725

    ADS  Google Scholar 

  • ten Brummelaar TA, McAlister HA, Ridgway ST, Bagnuolo WG, Turner NH, Sturmann L, Sturmann J, Berger DH, Ogden CE, Cadman R, Hartkopf WI, Hopper CH and Shure MA (2005). First Results from the CHARA Array. II. A Description of the Instrument. Astrophys J 628: 453–465

    Article  ADS  Google Scholar 

  • ten Brummelaar TA, McAlister HA, Ridgway ST, Turner NH, Sturmann L, Sturmann J, Bagnuolo WG, Jr., Shure MA (2003) An Update of the CHARA Array. In: Traub WA (ed) nterferometry for optical astronomy II, Proc. SPIE, vol 4838, p 69

  • Théado S, Vauclair S, Castro M, Charpinet S and Dolez N (2005a). Asteroseismic tests of element diffusion in solar type stars. Astron Astrophys 437: 553–560

    Article  ADS  Google Scholar 

  • Théado S, Vauclair S and Cunha MS (2005b). Helium settling and mass loss in magnetic Ap stars. I. The chemical stratification. Astron Astrophys 443: 627–641

    Article  ADS  Google Scholar 

  • Thévenin F and Idiart T (1999). Stellar Iron abundances: non-LTE effects. Astrophys J 521: 753–763

    Article  ADS  Google Scholar 

  • Thévenin F, Provost J, Morel P, Berthomieu G, Bouchy F and Carrier F (2002). Asteroseismology and calibration of alpha Cen binary system. Astron Astrophys 392: L9–L12

    Article  ADS  Google Scholar 

  • Thévenin F, Kervalla P, Pichon B, Morel P, Di Folco E and Lebreton Y (2005). VLTI/VINCI diameter constraints on the evolutionary status of δ Eri, ξ Hya, η Boo. Astron Astrophys 436: 253–262

    Article  ADS  Google Scholar 

  • Thompson MJ and Christensen-Dalsgaard J (2002). On inverting asteroseismic data. In: Favata, F, Roxburgh, IW and Galadí-Enríquez, D (eds) Proc, 1st Eddington workshop, ‘stellar structure and habitable planet finding’, ESA SP-485, pp 95–101. ESA Publications Division, Noordwijk

    Google Scholar 

  • Thompson MJ, Christensen-Dalsgaard J, Miesch MS and Toomre J (2003). The internal rotation of the Sun. Annu Rev Astron Astrophys 41: 599–643

    Article  ADS  Google Scholar 

  • Thoul A, Scuflaire R, Noels A, Vatovez B, Briquet M, Dupret MA and Montalbán J (2003). A new seismic analysis of Alpha Centauri. Astron Astrophys 402: 293–297

    Article  ADS  Google Scholar 

  • Thoul A, Ausseloos M, Barban C, Briquet M, Bourge PO, Cuypers J, Daszynska K, De Cat P, De Ridder J, Dupret MA, Montalban J, Noels A, Scuflaire R, Uytterhoeven K and Aerts C (2003). A hare and hound in a BAG. Asteroseismology of β Cephei stars. Comm Asteroseismol 143: 25–28

    ADS  Google Scholar 

  • Tikhonov AN and Arsenin VA (1977). Solution of ill-posed problems. Winston, Washington

    Google Scholar 

  • Tomkin J and Fekel FC (2006). New precision orbits of bright double-lined spectroscopic binaries. I. RR Lyncis, 12 Bootis and HR 6169. Astron J 131: 2652–2663

    Article  ADS  Google Scholar 

  • Tomkin J, Pan X and McCarthy JK (1995). Spectroscopic detection of the secondaries of the Hyades interferometric spectroscopic binary theta2 Tauri and of the interferometric spectroscopic binary alpha Andromedae. Astrophys J 109: 780–790

    ADS  Google Scholar 

  • Torres G, Boden AF, Latham DW, Pan M and Stefanik RP (2002). Testing models of stellar evolution for metal-poor stars: an interferometric–spectroscopic orbit for the binary HD 195987. Astron J 124: 1716–1737

    Article  ADS  Google Scholar 

  • Townsend RHD (1997). Spectroscopic modelling of non-radial pulsation in rotating early-type stars. Mon Not R Astr Soc 284: 839–858

    ADS  Google Scholar 

  • Trampedach R, Christensen-Dalsgaard J, Nordlund Å and Stein RF (1998). Stellar background power spectra from hydrodynamical simulations of stellar atmospheres. In: Kjeldsen, H and Bedding, TR (eds) Proc. Workshop on science with a small space telescope, pp 59–67. Aarhus Universitet, Aarhus

    Google Scholar 

  • Traub WA (ed) (2003) Interferometry for optical astronomy II. Proc SPIE vol 4838, ISBN 9780819446176

  • Traub WA (ed) (2004) Interferometry for optical astronomy II. Proc SPIE 5491, ISBN 9780819454232

  • Tremblay PE, Fontaine G, Brassard P, Bergeron P and Randall SK (2006). A quantitative analysis of the available multicolor photometry for rapidly pulsating hot B subdwarfs. Astrophys J Suppl 165: 551–567

    Article  ADS  Google Scholar 

  • Turck-Chièze S, Couvidat S, Piau L, Ferguson J, Lambert P, Ballot J, García RA, Nghiem P (2004) Surprising Sun: a new step towards a complete picture? Phys Rev Lett 93:211102–(1–4)

    Google Scholar 

  • Ulrich RK (1970). The Five-Minute Oscillations on the Solar Surface. Astrophys J 162: 993–1002

    Article  ADS  Google Scholar 

  • Ulrich RK (1986). Determination of stellar ages from asteroseismology. Astrophys J 306: L37–L40

    Article  ADS  Google Scholar 

  • Ulrich RK (1986). Determination of stellar ages from asteroseismology. Mon Not R Astr Soc 330: 731–736

    Google Scholar 

  • Unno W (1967). The stellar radial pulsation coupled with the convection. Publ Astron Soc Jpn 19: 140–153

    ADS  Google Scholar 

  • Unno W, Osaki Y, Ando H, Saio H and Shibahashi H (1989). Nonradial oscillations of stars, 2nd edn. University of Tokyo Press, Tokyo

    Google Scholar 

  • Uytterhoeven K, Aerts C, De Cat P, De Mey K, Telting JH, Schrijvers C, De Ridder J, Daems K, Meeus G and Waelkens C (2001). Line–profile variations of the double-lined spectroscopic binary kappa Scorpii. Astron Astrophys 371: 1035–1047

    Article  ADS  Google Scholar 

  • Uytterhoeven K, Willems B, LefeverK Aerts C, Telting JH and Kolb U (2004a). Interpretation of the variability of the β Cephei star λ Scorpii. I. The multiple character. Astron Astrophys 427: 581–592

    Article  ADS  Google Scholar 

  • Uytterhoeven K, Telting JH, Aerts C and Willems B (2004b). Interpretation of the variability of the β Cephei star λ Scorpii. II. The line–profile diagnostics. Astron Astrophys 427: 593–605

    Article  ADS  Google Scholar 

  • Uytterhoeven K, Briquet M, Aerts C, Telting JH, Harmanec P, Lefever K and Cuypers J (2005). Disentangling component spectra of λ Scorpii, a spectroscopic binary with a pulsating primary. II. Interpretation of the line–profile variability. Astron Astrophys 432: 955–967

    Article  ADS  Google Scholar 

  • Vakili F, Percheron I (1991) On the Possibility to Detect NRP’s by Optical Interferometry. In: Baade D (ed) Rapid variability of OB-stars: nature and diagnostic value, ESO, p 77

  • van Belle GT, Lane BF, Thompson RR, Boden AF, Colavita MM, Dumont PJ, Mobley DW, Palmer D, Shao M, Vasisht GX, Wallace JK, Creech-Eakman MJ, Koresko CD, Kulkarni SR, Pan XP and Gubler J (1999). Radii and effective temperatures for G, K, and M giants and supergiants. Astron J 117: 521–533

    Article  ADS  Google Scholar 

  • van Belle G, Ciardi DR, Thompson RR, Akeson RL and Lada EA (2001). Altair’s oblateness and rotation velocity from long-baseline interferometry. Astrophys J 559: 1155–1164

    Article  ADS  Google Scholar 

  • van Belle GT, Ciardi DR, ten Brummelaar T, McAlister HA, Ridgway ST, Berger DH, Goldfinger PJ, Sturmann J, Sturmann L, Turner N, Boden AF, Thompson RR and Coyne J (2006). First results from the CHARA Array. III. Oblateness, rotational velocity, and gravity darkening of Alderamin. Astrophys J 637: 494–505

    Article  ADS  Google Scholar 

  • van Boekel R, Kervella P, Schöller M, Herbst T, Brandner W, de Koter A, Waters LBFM, Hillier DJ, Paresce F, Lenzen R and Lagrange AM (2003). Direct measurement of the size and shape of the present-day stellar wind of η Carinae. Astron Astrophys 410: L37–L40

    Article  ADS  Google Scholar 

  • van Boekel R, Min M, Leinert C, Waters LBFM, Richichi A, Chesneau O, Dominik C, Jaffe W, Dutrey A, Graser U, Henning Th, de Jong J, Köhler R, de Koter A, Lopez B, Malbet F, Morel S, Paresce F, Perrin G, Preibisch Th, Przygodda F, Schöller M and Wittkowski M (2004). The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks. Nature 432: 479–482

    Article  ADS  Google Scholar 

  • Vandakurov Yu V (1967) The frequency distribution of stellar oscillations. Astron Zh 44:786–797 (English translation: Soviet Astronomy AJ 11:630–638)

    Google Scholar 

  • Vauclair S and Théado S (2004). Asteroseismic signatures of helium gradients in main-sequence A stars, application to the roAp star HD 60435. Astron Astrophys 425: 179–185

    Article  ADS  Google Scholar 

  • Vio R, Strohmer T and Wamsteker W (2000). On the Reconstruction of Irregularly Sampled Time Series. Publ Astron Soc Pacific 112: 74–90

    Article  ADS  Google Scholar 

  • Viskum M, Kjeldsen H, Bedding TR, Dall TH, Baldry IK, Bruntt H and Frandsen S (1998). Oscillation mode identifications and models for the δ Scuti star FG Virginis. Astron Astrophys 335: 549–560

    ADS  Google Scholar 

  • van Neuman J and Wigner E (1929). Über merkwüdige diskrete Eigenwerte. Über das Verhalten von Eigenwerten bei adiabatischen Prozessen. Phys Z 30: 467–470

    Google Scholar 

  • von Zeipel H (1924). The radiative equilibrium of a rotating system of gaseous masses. Mon Not R Astr Soc 84: 665–683

    ADS  Google Scholar 

  • Waelkens C (1991). Slowly pulsating B stars. Astron Astrophys 246: 453–468

    ADS  Google Scholar 

  • Walker G, Matthews J, Kuschnig R, Johnson R, Rucinski S, Pazder J, Burley G, Walker A, Skaret K, Zee R, Grocott S, Carroll K, Sinclair P, Sturgeon D and Harron J (2003). The MOST asteroseismology mission: Ultraprecise photometry from space. Publ Astron Soc Pacific 115: 1023–1035

    Article  ADS  Google Scholar 

  • Walker GAH, Kuschnig R, Matthews JM, Reegen P, Kallinger T, Kambe E, Saio H, Harmanec P, Guenther DB, Moffat AFJ, Rucinski SM, Sasselov D, Weiss WW, Bohlender DA, Boži´c H, Hashimoto O, Koubský P, Mann R, Ruždjak D, Å koda P, Å lechta M, Sudar D, Wolf M and Yang S (2005a). Pulsations of the Oe Star ζ Ophiuchi from MOST satellite photometry and ground-based Spectroscopy. Astrophys J 623: L145–L148

    Article  ADS  Google Scholar 

  • Walker GAH, Kuschnig R, Matthews JM, Cameron C, Saio H, Lee U, Kambe E, Masuda S, Guenther DB, Moffat AFJ, Rucinski SM, Sasselov D and Weiss WW (2005b). MOST Detects g-Modes in the Be Star HD 163868. Astrophys J 635: L77–L80

    Article  ADS  Google Scholar 

  • Warner PB, Kaye AB and Guzik JA (2003). A theoretical γ Doradus instability strip. Astrophys J 593: 1049–1055

    Article  ADS  Google Scholar 

  • Watson RD (1988). Contributing factors to flux changes in nonradial stellar pulsations. Astrophys Space Sci 140: 255–290

    Article  ADS  Google Scholar 

  • Winget DE, Nather RE, Clemens JC, Provencal J, Kleinman SJ, Bradley PA, Wood MA, Claver CF, Frueh ML, Grauer AD, Hine BP, Hansen CJ, Fontaine G, Achilleos N, Wickramasinghe DD, Marar TMK, Seetha S, Ashoka BN, O’Donoghue D, Warner B, Kurtz DW, Buckley DA, Brickhill J, Vauclair G, Dolez N, Chevreton M, Barstow MA, Solheim JE, Kanaan A, Kepler SO, Henry GW and Kawaler SD (1991). Asteroseismology of the DOV star PG 1159–035 with the whole earth telescope. Astrophys J 378: 326–346

    Article  ADS  Google Scholar 

  • Winget DE, Nather RE, Clemens JC, Provencal JL, Kleinman SJ, Bradley PA, Claver CF, Dixson JS, Montgomery MH, Hansen CJ, Hine BP, Birch P, Candy M, Marar TMK, Seetha S, Ashoka BN, Leibowitz EM, O’Donoghue D, Warner B, Buckley DAH, Tripe P, Vauclair G, Dolez N, Chevreton M, Serre T, Garrido R, Kepler SO, Kanaan A, Augusteijn T, Wood MA, Bergeron P and Grauer AD (1994). Whole Earth telescope observations of the DBV white dwarf GD 358. Astrophys J 430: 839–849

    Article  ADS  Google Scholar 

  • Wittkowski M, Hummel CA, Johnston KJ, Mozurkewich D, Hajian AR and White NM (2001). Direct multi-wavelength limb-darkening measurements of three late-type giants with the Navy Prototype Optical Interferometer. Astron Astrophys 377: 981–993

    Article  ADS  Google Scholar 

  • Wittkowski M, Aufdenberg JP and Kervella P (2004). Tests of stellar model atmospheres by optical interferometry. VLTI/VINCI limb-darkening measurements of the M4 giant ψ Phe. Astron Astrophys 413: 711–723

    Article  ADS  Google Scholar 

  • Wittkowski M, Hummel CA, Aufdenberg JP and Roccatagliata V (2006). Tests of stellar model atmospheres by optical interferometry. III. NPOI and VINCI interferometry of the M0 giant γ Sagittae covering 5-2μm. Astron Astrophys 460: 843–853

    Article  ADS  Google Scholar 

  • Wittkowski M, Boboltz DA, Ohnaka K, Driebe T and Scholz M (2007). The Mira variable S Orionis: relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs. Astron Astrophys 470: 191–210

    Article  ADS  Google Scholar 

  • Wolff CL (1974). Distinctive patterns on the surface of slowly rotating stars whose oscillations are nonlinearly coupled. Astrophys J 193: 721–727

    Article  ADS  Google Scholar 

  • Wu Y (2001). Combination frequencies in the Fourier spectra of white dwarfs. Mon Not R Astr Soc 323: 248–256

    Article  ADS  Google Scholar 

  • Xiong DR and Deng L (2001). Turbulent convection and pulsational stability of variable stars. – IV. The red edge of the δ Scuti instability strip. Mon Not R astr Soc 324: 243–248

    Google Scholar 

  • Xiong DR, Chen QL and Deng L (1997). Nonlocal time-dependent convection theory. Astrophys J Suppl 108: 529–544

    Article  ADS  Google Scholar 

  • Xiong DR, Deng L and Cheng QL (1998). Turbulent convection and pulsational stability of variable stars. I. Oscillations of long-period variables. Astrophys J 499: 355–366

    Article  ADS  Google Scholar 

  • Yildiz M (2007). Models of α Centauri A and B with and without seismic constraints: time dependence of the mixing-length parameter. Mon Not R Astr Soc 374: 1264–1270

    Article  ADS  Google Scholar 

  • Zahn JP (1991). Convective penetration in stellar interiors. Astron Astrophys 252: 179–188

    ADS  Google Scholar 

  • Zhao M, Monnier JD, Torres G, Boden AF, Claret A, Millan-Gabet R, Pedretti E, Berger JP, Traub WA, Schloerb FP, Carleton NP, Kern P, Lacasse MG, Malbet F and Perraut K (2007). Physical orbit for λ Virginis and a test of stellar evolution models. Astrophys J 659: 626–641

    Article  ADS  Google Scholar 

  • Zhevakin SA (1953). K Teorii Cefeid. I (On the theory of Cepheids I) (in Russian). Astron Zh 30: 161–179

    Google Scholar 

  • Zhevakin SA (1963). Physical basis of the pulsation theory of variable stars. Annu Rev Astron Astrophys 1: 367–400

    Article  ADS  Google Scholar 

  • Zima W (2006). A new method for the spectroscopic identification of stellar non-radial pulsation modes. I. The method and numerical tests. Astron Astrophys 455: 227–234

    Article  ADS  Google Scholar 

  • Zima W, Wright D, Bentley J, Cottrell PL, Heiter U, Mathias P, Poretti E, Lehmann H, Montemayor TJ and Breger M (2006). A new method for the spectroscopic identification of stellar non-radial pulsation modes. II. Mode identification of the δ Scuti star FG Virginis. Astron Astrophys 455: 235–246

    Article  ADS  Google Scholar 

  • Zwahlen N, North P, Debernardi Y, Eyer F, Galland L, Groenewegen MAT and Hummel CA (2004). A purely geometric distance to the binary star Atlas, a member of the Pleiades. Astron Astrophys 425: L45–L48

    Article  ADS  Google Scholar 

  • Zwintz K, Weiss WW, Kuschnig R, Gruber R, Frandsen S, Gray R and Jenkner H (2000). Variable HST guide stars (I). Astron Astrophys Suppl 145: 481–490

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to M. S. Cunha.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Cunha, M.S., Aerts, C., Christensen-Dalsgaard, J. et al. Asteroseismology and interferometry. Astron Astrophys Rev 14, 217–360 (2007). https://doi.org/10.1007/s00159-007-0007-0

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00159-007-0007-0

keywords

Navigation