F型星中铍、锂与氧的丰度
天体物理学
2007-05-23 v1
摘要
推导了 F 型场星中铍和氧的丰度，既因这些星之前已测得锂的丰度，从而获得观测约束，以判别不同混合机制。与角动量输运相关的混合以及框架内的内部重力波，在旋转演化模型中，似乎是解释观测结果的有前景的途径。
引用
@article{arxiv.astro-ph/9710065,
title = {Beryllium, Lithium and Oxygen Abundances in F-type Stars},
author = {R. J. Garcia Lopez and M. C. Dominguez Herrera and M. R. Perez de Taoro and C. Casares and J. L. Rasilla and R. Rebolo and C. Allende Prieto},
journal= {arXiv preprint arXiv:astro-ph/9710065},
year = {2007}
}
备注
Latex file (8 pages), uses html.sty, epsf.sty and cs10.sty (included); 3 EPS figures. To appear in the Proceedings of the 10th Cambridge Workshop Cool Stars, Stellar Systems and the Sun (Cambridge, MA USA, July 1997)