Other
Scientific paper
Dec 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99.1288p&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, Dec. 1987, p. 1288-1291.
Other
48
Abundance, F Stars, Lithium, Open Clusters, Stellar Evolution, Stellar Spectra, Dwarf Stars, Main Sequence Stars, Nuclear Fusion, Spectrum Analysis, Stellar Spectrophotometry
Scientific paper
The abundance of lithium has been determined for 18 stars in the Pleiades cluster with spectral types from A7 V to G0 V. The pronounced dip in the lithium abundance among the mid-F stars which has been reported for other, older star clusters is not present in the Pleiades. The removal of lithium from the surfaces of middle-F dwarfs therefore occurs principally after about 108years on the main sequence.
Booth John
Hobbs Lew M.
Pilachowski Catherine A.
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