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].
@article{arxiv.astro-ph/9503009,
title = {Absolute-Magnitude Calibration for W~UMa-type Systems. II. Influence of Metallicity},
author = {Slavek Rucinski},
journal= {arXiv preprint arXiv:astro-ph/9503009},
year = {2016}
}
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one PS file containing text and 5 figs, packed with uufiles