The evolution of dark matter halos and deep galaxy counts

被引：0
|
作者：
Jameson, A [1 ]
Longair, M [1 ]
Blain, A [1 ]
机构：
[1] Univ Cambridge, Cavendish Astrophys Grp, Cambridge CB2 1TN, England
来源：
THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO | 1999年 / 165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：
Galaxy formation and evolution are investigated using a hierarchical clustering model. The model is based upon the Press-Schechter formalism and describes the distribution of dark halos and halo mergers. Simple assumptions are made to relate dark halos and luminous galaxies in order to model B- and K-band source counts, the B-band redshift distribution and the global star-formation history. The effect of including a star-formation efficiency, which fits far-infrared and submillimetre-wave data, is shown to give encouraging results.
引用
收藏
页码：346 / 351
页数：6
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