The growth of galaxies in cosmological Simulations

被引：0
|
作者：
Choi, JH [1 ]
Katz, N [1 ]
Murali, C [1 ]
Weinberg, D [1 ]
Davé, R [1 ]
Hernquist, L [1 ]
机构：
[1] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
来源：
NEW ERA IN COSMOLOGY | 2002年 / 283卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
What galaxies look like today clearly depends on how they were assembled. There are two ways that galaxies can gain mass: Smooth accretion of cooling or cool gas and merging with smaller galaxies. Here we compare the relative importance of smooth accretion and merging in the assembly of galaxies using a cosmological N-body/hydrodynamic simulation. We also investigate its dependence on environment.
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收藏
页码：343 / 345
页数：3
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