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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1792
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dc.contributor.authorLambert, D. L-
dc.contributor.authorReddy, B. E-
dc.date.accessioned2007-09-14T10:38:39Z-
dc.date.available2007-09-14T10:38:39Z-
dc.date.issued2005-09-
dc.identifier.citationAstronomical Society of the Pacific Conference Series, Vol. 336, pp. 347 - 350en
dc.identifier.urihttp://hdl.handle.net/2248/1792-
dc.descriptionRestricted Accessen
dc.description.abstractLithium abundances for a sample of 451 F and G dwarfs including 181 new stars all belonging to the Galactic thin disk are discussed. Lithium abundances, metallicities ([Fe/H]), masses, and ages are determined (Lambert & Reddy 2004). The field stars span a larger range in [Fe/H] than the open clusters for which [Fe/H] ≈ 0.0±0.2. The initial Li from which stars formed has been traced from stars for which astration of lithium is believed to be unimportant.en
dc.format.extent178094 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://aspbooks.org/custom/publications/paper/336-0347.htmlen
dc.subjectLi Abundance Surveyen
dc.titleLi Abundance Survey in Galactic Thin Disken
dc.typeArticleen
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