Physics and Gas Dynamics of Wind-Blown Bubbles

被引：0
|
作者：
S.A. Zhekov
A.V. Myasnikov
机构：
[1] JILA,
[2] University of Colorado,undefined
[3] Institute for problems in mechanics,undefined
来源：
Astrophysics and Space Science | 2000年 / 274卷
关键词：
Massive Star; Stellar Wind; Contact Discontinuity; Stellar Evolution; Central Star;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We review the recent hydrodynamic modelling of wind-blown bubbles (WBB) which are result of interaction of a stellar wind with the circumstellar matter or the wind(s) emitted during the previous stages of the central star evolution. The much faster computers becoming available in the last decade allow a more complete picture of the physics of these objects to be built. Recent hydrodynamic models are capable of treating in detail different mechanisms as radiative plasma cooling, electron thermal conduction and the effects of magnetic fields. We discuss the various mechanisms proposed for shaping these objects and we emphasize on the problems related to the development of various instabilities and the X-ray emission from WBB.
引用
收藏
页码：243 / 255
页数：12
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