Collisional dynamics of black holes, star clusters and galactic nuclei

被引:0
|
作者
Khalisi, E [1 ]
Omarov, C [1 ]
Spurzem, R [1 ]
Giersz, M [1 ]
Lin, DNC [1 ]
机构
[1] Astron Rech Inst, D-69120 Heidelberg, Germany
来源
HIGH PERFORMANCE COMPUTING IN SCIENCE AND ENGINEERING'03 | 2003年
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D O I
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use high-precision direct N-body integration to study questions of the thermodynamic behaviour of dense stellar systems. The processes examined include mass segregation and equipartition processes, the study of planetary orbits in dense star clusters, and stellar orbits in galactic nuclei with thick accretion disks.
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收藏
页码:71 / 87
页数:17
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