Relativistic low angular momentum accretion in 3D

被引：0
|
作者：
Sukova, Petra [1 ]
Charzynski, Szymon [1 ,2 ]
Janiuk, Agnieszka [1 ]
机构：
[1] Ctr Theoret Phys PAS, Al Lotnikow 32-46, PL-02668 Warsaw, Poland
[2] Univ Warsaw, Chair Math Methods Phys, Ul Pasteura 5, PL-02093 Warsaw, Poland
来源：
XXXVII POLISH ASTRONOMICAL SOCIETY MEETING | 2016年 / 3卷
关键词：
FLOW;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study the low angular momentum accretion of matter onto Schwarzschild or Kerr black hole using fully relativistic numerical simulations. Our aim is to include the rotation of both the gas and the black hole and the presence of the magnetic field into the picture. We compare resulting structure of transonic flow with results of 1D pseudo-Newtonian semi-analytical computations of non-magnetized flow.
引用
收藏
页码：150 / 153
页数：4
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