Light Elements in Main Sequence Stars: Li, Be, B, C, O
Abstract
The abundances of the 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 abundant light elements, C and O, reveal information about the chemical history of the Galaxy and the mass spectrum of early generations of stars.
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