Selfconsistent models of winds from rotating early-type stars - Application to B[e] star winds

被引：0
|
作者：
Petrenz, P [1 ]
Puls, J [1 ]
机构：
[1] Univ Munich, Inst Astron & Astrophys, D-81679 Munich, Germany
来源：
BE PHENOMENON IN EARLY-TYPE STARS, PROCEEDINGS | 2000年 / 175卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present results of 2.5-D radiation hydrodynamical simulations of winds from rapidly rotating stars. For the first time, we consider the dependence of the line statistics on local density and radiation temperature implying a spatial variation of the force-multiplier parameters k, alpha and delta which control the dynamics of the flow. We apply our models to the problem of disk formation in B[e]-star winds.
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页码：626 / 631
页数：2
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