X-rays from A stars - Coronae and wind-shocks

被引：0
|
作者：
Robrade, J. [1 ]
机构：
[1] Univ Hamburg, Hamburger Sternwarte, Hamburg, Germany
来源：
PUTTING A STARS INTO CONTEXT: EVOLUTION, ENVIRONMENT, AND RELATED STARS | 2014年
关键词：
CHEMICALLY PECULIAR STARS; DRIVEN STELLAR WINDS; DYNAMICAL SIMULATIONS; BETA-PICTORIS; EMISSION; ALTAIR; MODEL;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The X-ray properties of A stars are reviewed and their X-ray generating mechanisms discussed. A-type stars bridge the regimes of cool and hot stars and exhibit diverse high-energy features; in particular, among A stars are found the hottest magnetically active stars as well as the coolest wind-shock stars. In the domain of late A-type stars X-ray emission is related to the presence of coronae, while in Ap/Bp stars a magnetically channelled wind-shock model is applicable.
引用
收藏
页码：425 / 434
页数：10
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