The gravity-darkening of highly distorted stars in close binary systems. V - Practical analysis of the contact components of W Ursa Majoris-type systems

Astronomy and Astrophysics – Astrophysics

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Darkening, Eclipsing Binary Stars, Stellar Spectrophotometry, Light Curve, Roche Limit, Stellar Mass, Stellar Temperature

Scientific paper

A quantitative analysis of the photometric ellipticity effect has been performed in order to obtain values of the exponent of gravity-darkening (alpha) for the components of 16 W UMa systems. For the case in which the fill-out factors are less than 0.5, the alpha values are found to be greater than the conventional value of 0.32. The results suggest that the structure of the photosphere of W UMa contact components is significantly different from that of normal Main-Sequence stars of similar spectral type.

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