中间质渐进巨星分支星的核合成
天体物理学
2007-05-23 v1
摘要
我们概述了渐进巨星分支(AGB)星的主要特性，包括其结构、演化与核合成过程。阐述了主要的物理机制及其不确定性。鉴于本次会议的多学科性质，这篇论文面向那些并非星体结构专家的读者。
引用
@article{arxiv.astro-ph/9810094,
title = {Nucleosynthesis in Intermediate-Mass Asymptotic Giant Branch Stars},
author = {John C. Lattanzio},
journal= {arXiv preprint arXiv:astro-ph/9810094},
year = {2007}
}
备注
7 pages, 3 figures, Invited Review presented at Nuclei in the Cosmos V, Volos, July 1998. For non-experts in stellar strucure! For related papers please see http://www.maths.monash.edu.au/~johnl/