中间质量星的热脉冲AGB模型
天体物理学
2007-05-23 v1
摘要
我们present了一组初始质量大于5太阳质量的AGB星模型，这些模型使用FRANEC代码计算得出。包括Z=0.02和Z=0.001的模型，分别考虑有无质量损失的情况。
引用
@article{arxiv.astro-ph/9912426,
title = {Thermally Pulsing AGB Models of Intermediate Mass Stars},
author = {O. Straniero and M. Limongi and A. Chieffi and I. Dominguez and M. Busso and R. Gallino},
journal= {arXiv preprint arXiv:astro-ph/9912426},
year = {2007}
}
备注
9 pages, 9 figures (memsait.sty, epsf.sty) contribution to the workshop "The Changes in Abundances in Asymptotic Giant Branch Stars", held in Monte Porzio Catone (Italy), September 1999, to be published by Mem.Soc.Astron.It., eds. F. D'Antona and R. Gallino