Multicomponent stellar wind from hot subdwarfs stars

被引：0
|
作者：
V. Votruba
A. Feldmeier
J. Krtička
J. Kubát
机构：
[1] Akademie věd České Republiky,Astronomický Ústav
[2] Universität Potsdam,Astrophysik, Institut für Physik
[3] Masarykova Univerzita,Ústav Teoretické Fyziky a Astrofyziky, Přírodověcká Fakulta
来源：
Astrophysics and Space Science | 2010年 / 329卷
关键词：
Stellar wind; Hot subdwarfs; Decoupling;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Stellar wind from hot subdwarf stars is mainly accelerated by the interaction of ultraviolet photospheric radiation with metals, mainly oxygen. Absorbing ions share momentum through Coulombic collisions with the remaining passive part of the plasma (namely protons). We found that in the case of the winds from hot subdwarfs, interactions could be so small that they stop the momentum transfer between the passive bulk of plasma and absorbing ions. As a result wind decouples at a certain point.
引用
收藏
页码：159 / 161
页数：2
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