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Absolute-Magnitude Calibration for W~UMa-type Systems. II. Influence of Metallicity

Slavek Rucinski

astro-pharXiv:astro-ph/9503009

Abstract

A modification to the absolute magnitude calibration for W~UMa-type systems, taking into account differences in metal abundances, is derived on the basis of contact binary systems recently discovered in metal-poor clusters. A preliminary estimate of the magnitude of the metallicity-dependent term for the (B-V)-based calibration is ΔMV = -(0.3 0.1) × [Fe/H]. The calibration based on the (V-IC) color is expected to be less sensitive with the correction term ≈ -(0.12 0.05) × [Fe/H].

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