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The W UMa-type Stars Program: First Results, Current Status and Perspectives

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Abstract

We present the results of a statistical investigation of the period-color and period-bolometric magnitude relations using a carefully selected sample of 120 contact systems with known physical parameters.

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Authors and Affiliations

  1. Mt. Suhora Observatory, Cracow Pedagogical University, Cracow, Poland

    J. M. Kreiner, S. Zola, W. Ogloza, B. Pokrzywka, M. Drozdz, G. Stachowski & B. Zakrzewski

  2. Department of Astrophysics, Astronomy and Mechanics, Faculty of Physics, University of Athens, Athens, Greece

    P. G. Niarchos & K. Gazeas

  3. David Dunlap Observatory, University of Toronto, Toronto, Canada

    S. M. Rucinski

  4. Astronomical Observatory of the Jagiellonian University, Cracow, Poland

    M. Siwak & D. Koziel

  5. Department of Physics, Shoumen University, Shoumen, Bulgaria

    D. Kjurkchieva & D. Marchev

Authors
  1. J. M. Kreiner
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  2. S. Zola
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  3. W. Ogloza
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  4. B. Pokrzywka
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  5. M. Drozdz
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  6. G. Stachowski
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  7. B. Zakrzewski
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  8. P. G. Niarchos
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  9. K. Gazeas
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  10. S. M. Rucinski
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  11. M. Siwak
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  12. D. Koziel
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  13. D. Kjurkchieva
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  14. D. Marchev
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Kreiner, J.M., Zola, S., Ogloza, W. et al. The W UMa-type Stars Program: First Results, Current Status and Perspectives. Astrophys Space Sci 304, 71–73 (2006). https://doi.org/10.1007/s10509-006-9077-0

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  • DOI: https://doi.org/10.1007/s10509-006-9077-0

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