Solar-like oscillations

被引：119
|
作者：
Bedding, TR [1 ]
Kjeldsen, H
机构：
[1] Univ Sydney, Sch Phys A28, Sydney, NSW 2006, Australia
[2] Danmarks Grundforskningsfond, Teoretisk Astrofys Ctr, DK-8000 Aarhus C, Denmark
[3] Inst Fys & Astron, DK-8000 Aarhus C, Denmark
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2003年 / 20卷 / 02期
关键词：
stars; oscillations;
D O I：
10.1071/AS03025
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The five-minute oscillations in the Sun have provided a wealth of information about the solar interior. After many attempts, positive detections of similar oscillations in solar-type stars have now been made. This review discusses the properties of solar-like oscillations, the methods used to observe them, and the results on individual stars. We conclude that the study of solar-like oscillations from the ground and space has an exciting future.
引用
收藏
页码：203 / 212
页数：10
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