Formation and evolution of galactic nuclei, black holes

被引：1
|
作者：
Spurzem, R [1 ]
机构：
[1] Astron Rech Inst, D-69120 Heidelberg, Germany
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2003年 / 284卷 / 02期
关键词：
galactic nuclei; black holes; numerical methods;
D O I：
10.1023/A:1024041519207
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The formation and evolution of galactic nuclei is discussed, mainly from the viewpoint of the dense gaseous and stellar system in the central portions of young galactic nuclei. A review is given on models of galactic nuclei containing one or more black holes and how the standard historic Rees-Spitzer-Stone scenario of isolated nuclei formation has been changed by the cosmological structure formation scenario. The dynamical interaction of two or more black holes with their stellar environment and their merging possibilities is presented.
引用
收藏
页码：551 / 559
页数：9
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