Light Elements in Main Sequence Stars: Li, Be, B, C, O

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dc.creatorBoesgaard, Ann Merchant
dc.date2004-12-09
dc.date.accessioned2026-07-07T02:16:10Z
dc.date.available2026-07-07T02:16:10Z
dc.descriptionThe abundances of the {\it rare} light elements, Li, Be, and B, provide clues about stellar structure and evolution, about Galactic evolution and about their nucleosynthesis, including production during the Big Bang. The abundances of the {\it abundant} light elements, C and O, reveal information about the chemical history of the Galaxy and the mass spectrum of early generations of stars.
dc.descriptionPaper for Lambert Symposium: "Cosmic Abundances as records of Stellar Evolution and Nucleosynthesis" 14 pages, 15 figures, 1 table
dc.identifierhttps://arxiv.org/abs/astro-ph/0412198
dc.identifierhttp://arxiv.org/abs/astro-ph/0412198
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8689
dc.subjectAstrophysics
dc.titleLight Elements in Main Sequence Stars: Li, Be, B, C, O
dc.typetext

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