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
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：
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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页码：71 / 87
页数：17
相关论文
共 46 条
[1]   Star cluster simulations: The state of the art [J].
Aarseth, SJ .
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 1999, 73 (1-4) :127-137
[2]   From NBODY1 to NBODY6: The growth of an industry [J].
Aarseth, SJ .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1999, 111 (765) :1333-1346
[3]   STAR TRAPPING AND METALLICITY ENRICHMENT IN QUASARS AND ACTIVE GALACTIC NUCLEI [J].
ARTYMOWICZ, P ;
LIN, DNC ;
WAMPLER, EJ .
ASTROPHYSICAL JOURNAL, 1993, 409 (02) :592-603
[4]  
BISNOVATYIKOGAN GS, 1978, ASTRON LETT+, V4, P130
[5]  
DAVIES MB, 1998, MNRAS, V295, P691
[6]  
DELAFUENTE MC, 1998, NEW ASTRON, V4, P21
[7]  
DELAFUENTE MC, 1997, ASTRON ASTROPHYS, V326, pL21
[8]   A stochastic Monte Carlo approach to model real star cluster evolution - II. Self-consistent models and primordial binaries [J].
Giersz, M ;
Spurzem, R .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2000, 317 (03) :581-606
[9]   STATISTICS OF N-BODY SIMULATIONS .1. EQUAL MASSES BEFORE CORE COLLAPSE [J].
GIERSZ, M ;
HEGGIE, DC .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1994, 268 (01) :257-275
[10]  
GIERSZ M, 2003, IN PRESS MNAS
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