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- W58252870 abstract "Abstract We present results based on the analysis of lithium abundances in a sample of ~ 50 pre-main sequence stars covering a wide range of masses (from 2 to 0.3 M ⊙ ) and luminosities (corresponding to ages of 1-100 Myr). Stars with masses estimated to be ≳ 1 M ⊙ show lithium abundances close to cosmic with little scatter (± 0.3 dex). Stars with masses less than Solar present a wide range of lithium abundances, with a clear trend to lower abundances for lower luminosities (greater age). The observed Li abundances constrain theoretical predictions of lithium depletion in rotating pre-main sequence stars." @default.
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- W58252870 date "1993-01-01" @default.
- W58252870 modified "2023-10-18" @default.
- W58252870 title "Observational Patterns of Lithium Depletion in Pre-Main Sequence Stars" @default.
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- W58252870 doi "https://doi.org/10.1017/s025292110001767x" @default.
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