Asteroseismology of solar-type stars: particular physical effects

被引：4
|
作者：
Carrier, F. [1 ]
Eggenberger, P. [2 ]
Leyder, J. -C [2 ]
机构：
[1] Katholieke Univ Leuven, Inst Sterrenkunde, Celestijnenlaan 200D, B-3001 Louvain, Belgium
[2] Univ Liege, Inst Astrophys & Geophys, B-4000 Liege, Belgium
来源：
PROCEEDINGS OF THE SECOND HELAS INTERNATIONAL CONFERENCE: HELIOSEISMOLOGY, ASTEROSEISMOLOGY AND MHD CONNECTIONS | 2008年 / 118卷
基金：
瑞士国家科学基金会;
关键词：
D O I：
10.1088/1742-6596/118/1/012047
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Since the success of helioseismology, numerous efforts have been made to detect solar-like oscillations on other stars. The measurement of the frequencies of p-mode oscillations provides an insight into the internal structure and is nowadays the most powerful constraint on the theory of stellar evolution. The existing asteroseismic observations were mainly motivated by the need to explore the seismological properties of stars with various global parameters, i.e. various locations in the HR diagram. With the aim of testing different physical effects on solar-like oscillations, we report here detection of acoustic modes on solar-like targets achieved with the spectrograph HARPS installed on the 3.6-m telescope at ESO La Silla Observatory.
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页数：5
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