Light Elements in Main Sequence Stars: Li, Be, B, C, O
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/0412198,
title = {Light Elements in Main Sequence Stars: Li, Be, B, C, O},
author = {Ann Merchant Boesgaard},
journal= {arXiv preprint arXiv:astro-ph/0412198},
year = {2007}
}
Comments
Paper for Lambert Symposium: "Cosmic Abundances as records of Stellar Evolution and Nucleosynthesis" 14 pages, 15 figures, 1 table