arXiv · astro-ph/9503009
Absolute-Magnitude Calibration for W~UMa-type Systems. II. Influence of Metallicity
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 $ΔM_V = -(0.3 \pm 0.1) \times [Fe/H]$. The calibration based on the $(V-I_C)$ color is expected to be less sensitive with the correction term $\approx -(0.12\pm 0.05) \times [Fe/H]$.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Slavek Rucinski. 1995-03-01. Absolute-Magnitude Calibration for W~UMa-type Systems. II. Influence of Metallicity. https://doi.org/10.1086/133603
Cite the original work for its findings. Save a collection to share your selection of sources.