银河系盘的构建与演化
天体物理学
2007-05-23 v1
摘要
在宇宙学背景下研究盘状星系的形成与演化。我们考察盘状星系的可观测属性，自洽地处理盘的形成与星系演化过程。我们发现，决定哈伯序列的主要因素是物质吸积方式。这种吸积方式直接与盘状星系所起源的原始密度涨落的统计特性相关。本文采用高斯密度场和标准 CDM 模型。
引用
@article{arxiv.astro-ph/9610046,
title = {The Building up and Evolution of Galactic Disks},
author = {Claudio Firmani and Vladimir Avila-Reese and Xavier Hernández},
journal= {arXiv preprint arXiv:astro-ph/9610046},
year = {2007}
}
备注
Presented at the Conference "Dark and Visible Matter in Galaxies and Cosmological Implications" (Sesto, Italy, 2-5 July 1996), to appear in A.S.P. Conference Series, 7 pages, 4 figures, Latex, uses paspconf.sty, epsf.sty