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On the Gravity Darkening of Eclipsing Variables of W UMa Type

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Part of the book series: NATO Science Series ((ASIC,volume 544))

Abstract

The theoretical and observational methods for the determination of the gravity darkening exponents in contact binaries of W UMa type are briefly presented. Among the theoretical ones, those of von Zeipel, Lucy and Claret are given special attention. The results of observational approaches developed by several investigators are also presented and discussed.

The main points of a new method for the determination of the gravity darkening in W UMa systems are presented. It is based on Kopal’s method of Fourier analysis of the light changes of eclipsing variables in the Frequency Domain. The method is applied to a large enough sample of W UMa systems for which geometric and photometric elements have been derived by the most powerful techniques. The results of the new method confirm the previous ones with the assumed, same geometrical parameters. The derived values are very close to those predicted by the existing theory of radiative transfer or convective equilibrium.

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1The present work is dedicated to the memory of Professor Z. Kopal

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© 2000 Springer Science+Business Media Dordrecht

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Niarchos, P.G. (2000). On the Gravity Darkening of Eclipsing Variables of W UMa Type. In: İbanoğlu, C. (eds) Variable Stars as Essential Astrophysical Tools. NATO Science Series, vol 544. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4299-1_34

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  • DOI: https://doi.org/10.1007/978-94-011-4299-1_34

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-6084-1

  • Online ISBN: 978-94-011-4299-1

  • eBook Packages: Springer Book Archive

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