INVESTIGATION OF STABILITY OF BONDI-HOYLE MODEL OF ACCRETION FLOW

被引:32
作者
COWIE, LL [1 ]
机构
[1] HARVARD UNIV,DEPT PHYS,CAMBRIDGE,MA 02138
关键词
Accretion flow - Moving body - Short wavelengths - Steady state solution;
D O I
10.1093/mnras/180.4.491
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have reinvestigated the Bondi-Hoyle-Lyttleton model of gravitational accretion on to fast-moving bodies. The stability of the steady state solution has been analysed and the accretion column shown to be unstable against short-wavelength perturbations. © Royal Astronomical Society.
引用
收藏
页码:491 / 494
页数:4
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