年轻恒星团周围气体的状态
天体物理学
2007-05-23 v1
摘要
我们描述了恒星形成区气体压力演化的主要特征,从母云形成到区域被相互作用的恒星风压制为止。描述了云的破坏过程及星形成的自限制特性。高效率的星形成是由于高气体压力所致。也勾勒了高度压制区域中缓慢风的演化。
引用
@article{arxiv.astro-ph/9609054,
title = {The State of the Gas Around Young Stellar Groups},
author = {J. Franco and T. Plewa and G. Garcia-Segura},
journal= {arXiv preprint arXiv:astro-ph/9609054},
year = {2007}
}
备注
5 pages, latex, uses rmaaconf.sty, 1 figure (included); also available at http://www.mpa-garching.mpg.de/Hydro/AMR/papers/schyda.uu To appear in Rev. Mex. Astr. Astrofis. (1996), proceedings of the conference "Starburst Activity in Galaxies", ed. J. Franco, R. Terlevich, and G. Tenorio-Tagle