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M - L relations for rapid and slow rotators

Published online by Cambridge University Press:  01 August 2006

Oleg Yu. Malkov
Oleg Yu. Malkov*
Affiliation:
Center for Astronomical Data, Institute of Astronomy of the Russian Academy of Sciences, Pyatnitskaya ul. 48, 119017 Moscow, Russian Federation email: malkov@inasan.ru
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Abstract

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Comparing the radii of eclipsing binaries components and single stars we have found a noticeable difference between observational parameters of B0V - G0V components of eclipsing binaries and those of single stars of the corresponding spectral type. This difference was confirmed by re-analyzing the results of independent investigations published in the literature.

Keywords

binaries: eclipsing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 213
Copyright
Copyright © International Astronomical Union 2007