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- W2061954710 abstract "Using a non-local stellar convection theory for chemically inhomogeneous stars, we have calculated the lithium and beryllium depletions in mainsequence models of 0.7-1.15 M⊙ and have compared them with the observed depletions in open clusters of different ages. The results show that the general properties of lithium depletion in late type main-sequence stars with Teff < 5900K can be reproduced by convective overshooting mixing. We conclude that convective overshooting could be an important mechanism for the lithium depletion observed in late-type dwarfs." @default.
- W2061954710 created "2016-06-24" @default.
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- W2061954710 date "2007-07-01" @default.
- W2061954710 modified "2023-09-23" @default.
- W2061954710 title "Lithium and Beryllium Depletions in Late-type Main-sequence Stars" @default.
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- W2061954710 doi "https://doi.org/10.1016/j.chinastron.2007.06.010" @default.
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