Star cluster dynamics in galaxies

被引：0
作者：
Bekki, Kenji [1 ]
机构：
[1] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
来源：
STAR CLUSTERS: BASIC GALACTIC BUILDING BLOCKS THROUGHOUT TIME AND SPACE | 2010年 / 266期
关键词：
globular clusters: general; open clusters and associations: general; galaxies: formation; galaxies: evolution; SELF-CONSISTENT SIMULATIONS; LARGE-MAGELLANIC-CLOUD; GLOBULAR-CLUSTERS; EVOLUTION; FRICTION; SYSTEMS;
D O I：
10.1017/S1743921309991086
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
I present a review of star cluster (SC) dynamics in galaxies, with special emphasis on the effects of global galactic dynamics on SC formation and evolution. I particularly discuss (i) dynamical friction processes affecting SCs in galaxies of different masses, (ii) formation of stellar galactic nuclei and massive globular clusters (GCs) through multiple merging of SCs, (iii) interactions between giant molecular clouds (GMCs) and SCs; (iv) SC destruction due to the strong tidal fields in galaxy mergers and (v) the formation of low-mass dwarfs from numerous SCs. I also discuss some recent observational results on SC mass functions in dwarf galaxies and physical properties of GC systems in luminous galaxies based on recent results of numerical simulations of SC dynamics in galaxies.
引用
收藏
页码：219 / 230
页数：12
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