Solar-like oscillations

被引：120

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

页码：203 / 212

页数：10

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