Galaxy evolution: Inhomogeneous halo collapse

被引：0
|
作者：
Myers, JM [1 ]
Hartmann, DH [1 ]
The, LS [1 ]
机构：
[1] Clemson Univ, Clemson, SC 29634 USA
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2003年 / 284卷 / 02期
关键词：
galaxies : evolution; galaxies : formation; galaxies : globular clusters;
D O I：
10.1023/A:1024025323885
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In an effort to study the halo globular clusters we perform a simulation of inhomogeneous halo collapse using a SPH/N-body code. We include dark matter particles, ( cooling) gas, and stars. Supernova feedback is included as a heat source for the gas in the local environment of star forming regions. We find this model cannot reproduce the age distribution and spatial distribution of halo globular clusters.
引用
收藏
页码：787 / 790
页数：4
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