辐射反馈与星际气体云的光子蒸发
天体物理学
2007-05-23 v1
摘要
首次从暗淡中性星际介质（IGM）中凝结出的致 ionizing 辐射源，会产生向外扩展的离子化前沿，征服其周围环境，抢夺其他原始气体云，并光子蒸发它们。本文报告了首次对这一过程进行气体动力学模拟的结果，包括辐射传递，并给出一些观测诊断。
引用
@article{arxiv.astro-ph/9804117,
title = {Radiative Feedback and the Photoevaporation of Intergalactic Clouds},
author = {Paul R. Shapiro and Alejandro C. Raga and Garrelt Mellema},
journal= {arXiv preprint arXiv:astro-ph/9804117},
year = {2007}
}
备注
7 pages, 6 figures. One LaTeX file, one LaTeX style file, 6 postscript files, tar-ed and gzip-ed. To appear in Proceedings of the Workshop on H_2 in the Early Universe, eds. F. Palla, E. Corbelli, and D. Galli, Memorie Della Societa Astronomica Italiana, in press (1998)