Other
Scientific paper
May 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...373..250d&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 373, May 20, 1991, p. 250-253.
Other
31
Abundance, Lithium, Metallicity, Pre-Main Sequence Stars, Stellar Atmospheres, T Tauri Stars, Atmospheric Models, Line Spectra, Stellar Spectra
Scientific paper
The Li abundance of the T Tauri star BP Tau is determined from both the Li I 6707 and 6103 features, using high-accuracy observations and recent model atmospheres. Other work, based solely on analysis of the 6707 line, has found very high Li abundances in T Tauri stars. A significant difference is found between the abundances derived from the two different lines and no evidence in this star of a Li abundance significantly in excess of the typical Population I value log n(Li) about 3.0.
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