Asteroseismology: From dream to reality

被引:7
作者
Kurtz, DW [1 ]
机构
[1] Univ Cent Lancashire, Ctr Astrophys, Preston PR1 2HE, Lancs, England
[2] Observ Midi Pyrenees, Astrophys Lab, F-31400 Toulouse, France
关键词
D O I
10.1023/B:SOLA.0000031383.23996.ae
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
With the resounding success of helioseismology in determining the interior structure and rotation of the Sun, and in providing unprecedented studies of the interaction of pulsation and magnetic fields in the solar atmosphere, astronomers have been delighted, after decades of disappointing attempts, with the recent discovery of solar-like oscillations in xi Hya, beta Hyi, alpha CenA and B, eta Boo, nuInd, zeta Her, delta Eri, HD 20794, HD 160191, and others as this list is growing rapidly. There is now true seismology of some solar-like stars. Asteroseismology also studies stars with a wide variety of interior and surface conditions. For two decades asteroseismic techniques have been applied to many pulsating stars across the HR diagram. This review describes some recent developments for some selected classes of pulsating stars other than the solar-like oscillators.
引用
收藏
页码:123 / 135
页数:13
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