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• W2149449462 abstract "Context. Models of stellar structure and evolution can be constrained by measuring accurate parameters of detached eclipsing binaries in open clusters. Multiple binary stars provide the means to determine helium abundances in these old stellar systems, and in turn, to improve age estimates." @default.
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• W2149449462 date "2010-11-26" @default.
• W2149449462 modified "2023-09-26" @default.
• W2149449462 title "Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members" @default.
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• W2149449462 doi "https://doi.org/10.1051/0004-6361/201015503" @default.
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