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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1977年 / 180卷 / 03期

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

页码：491 / 494

页数：4

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