Non-radial pulsations in be stars

被引：0
|
作者：
Briot, D [1 ]
机构：
[1] Observ Paris, F-75014 Paris, France
来源：
STELLAR STRUCTURE AND HABITABLE PLANET FINDING | 2004年 / 538卷
关键词：
stars : emission-line; Be stars : oscillations;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Be stars (i.e. stars with emission lines) represent nearly 20% of B stars. Non-radial pulsations in Be stars were discovered more than twenty years ago and asteroseismology is the only way to study the internal structure of these stars. It may also provide clues to understand the so far unexplained formation of their circumstellar envelopes in which emission originates. A review of results obtained is presented; as well as future progress expected from Eddington observations.
引用
收藏
页码：289 / 291
页数：3
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