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Inner radii of dust shells and stellar diameters obtained by an infrared stellar interferometer at 11 micron wavelength

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Abstract

Visibility data and analyses are discussed for 16 late-type stars observed with the Infrared Spatial Interferometer (ISI) of the University of California, Berkeley.

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References

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Author notes

  1. L. J. Greenhill

    Present address: Center for Astrophysics, 60 Garden St., 02138, Cambridge, MA, USA

Authors and Affiliations

  1. Space Sciences Laboratory, University of California, 94720-7450, Berkeley, CA, USA

    W. C. Danchi, M. Bester, L. J. Greenhill, C. G. Degiacomi, N. Geis, D. Hale, B. Lopez & C. H. Townes

  2. I. Physikalisches Institut, Universität zu Köln, D-50937, Köln, Germany

    C. G. Degiacomi

  3. Physics Department, University of Pittsburgh, 15260, Pittsburgh, PA, USA

    D. Hale

  4. Observatoire de la Côte d'Azur, Nice cedex 4, 06304, France

    B. Lopez

Authors
  1. W. C. Danchi
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  2. M. Bester
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  3. L. J. Greenhill
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  4. C. G. Degiacomi
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  5. N. Geis
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  6. D. Hale
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  7. B. Lopez
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  8. C. H. Townes
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Danchi, W.C., Bester, M., Greenhill, L.J. et al. Inner radii of dust shells and stellar diameters obtained by an infrared stellar interferometer at 11 micron wavelength. Astrophys Space Sci 224, 447–448 (1995). https://doi.org/10.1007/BF00667898

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  • DOI: https://doi.org/10.1007/BF00667898

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