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• W2078585535 abstract "Context.Because of the lack of precise masses, the coverage of the main-sequence empirical mass-luminosity relation for stars in the mass range from 0.6 to 0.9 is incomplete. The nearby K-type visual and spectroscopic binary GJ 765.2 = MLR 224 is a good candidate for new reliable points in this significant part of the relation." @default.
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• W2078585535 date "2007-01-02" @default.
• W2078585535 modified "2023-10-17" @default.
• W2078585535 title "Accurate masses of low mass stars GJ 765.2AB (0.83 $mathcal{M}_{odot} +$ 0.76 $mathcal{M}_{odot}$)" @default.
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• W2078585535 doi "https://doi.org/10.1051/0004-6361:20066224" @default.
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