The structure of winds in AGB stars

被引：0
作者：
Elitzur, M [1 ]
Ivezic, Z [1 ]
Vinkovic, D [1 ]
机构：
[1] Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA
来源：
MASS-LOSING PULSATING STARS AND THEIR CIRCUMSTELLAR MATTER: OBSERVATIONS AND THEORY | 2003年 / 283卷
关键词：
stars : AGB and post-AGB; mass-loss; winds; outflows; dust; hydrodynamics; radiative transfer;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Most dusty winds are described by a set of similarity functions of a single independent variable that can be chosen as TV, the overall optical depth at visual. The self-similarity implies general scaling relations among the system parameters, in agreement with observations. Dust drift through the gas has a major impact on the structure of most winds.
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页码：265 / 273
页数：9
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