Stellar capture by an accretion disc

被引：14
|
作者：
Vokrouhlicky, D
Karas, V
机构：
[1] Charles Univ Prague, Astron Inst, CZ-18000 Prague, Czech Republic
[2] Observ Cote Azur, Dept CERGA, F-06130 Grasse, France
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1998年 / 293卷 / 01期
关键词：
accretion; accretion discs; celestial mechanics; stellar dynamics; stars; kinematics; galaxies; nuclei;
D O I：
10.1046/j.1365-8711.1998.01213.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The long-term evolution of a stellar orbit captured by a massive galactic centre via successive interactions with an accretion disc has been examined. An analytical solution describing the evolution of the stellar orbital parameters during the initial stage of the capture has been found. Our results are applicable to thin Keplerian discs with an arbitrary radial distribution of density and a rather general prescription for the star-disc interaction. Temporal evolution is given in the form of quadrature which can be carried out numerically.
引用
收藏
页码：L1 / L5
页数：5
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