坍缩与喷流：星际形成综合理论的进展
天体物理学
2007-05-23 v1
摘要
过去十年的观测进展揭示，星际形成与重力坍缩气体、双枢流和盘状结构的共存密切相关。两种星际形成理论分别认为恒星质量是由引力不稳定性决定，或由喷流冲刷掉初始奇异密度分布的坍缩包裹层决定。但两种观点都未能解释所有事实。本稿考察了星际形成理论面临的关键问题。
引用
@article{arxiv.astro-ph/9702232,
title = {Collapse and Outflow: Towards an Integrated Theory of Star Formation},
author = {R. E. Pudritz and D. E. McLaughlin and R. Ouyed},
journal= {arXiv preprint arXiv:astro-ph/9702232},
year = {2007}
}
备注
12 pages with 2 ps figures. Invited review to appear in Computational Astrophysics, Proceedings of the 12th Kingston Meeting, ed. D. A. Clarke and M. J. West (San Francisco: ASP)