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

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The 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.
Paper for Lambert Symposium: "Cosmic Abundances as records of Stellar Evolution and Nucleosynthesis" 14 pages, 15 figures, 1 table

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