Seismic Analysis of Four Solar-like Stars Observed during More Than Eight Months by Kepler

被引：0
|
作者：
Mathur, S. [1 ]
Campante, T. L.
Handberg, R.
Garcia, R. A.
Appourchaux, T.
Bedding, T. R.
Mosser, B.
Chaplin, W. J.
Ballot, J.
Benomar, O.
Bonanno, A.
Corsaro, E.
Gaulme, P.
Hekker, S.
Regulo, C.
Salabert, D.
Verner, G.
White, T. R.
Brandao, I. M.
Creevey, O. L.
Dogan, G.
Bazot, M.
Cunha, M. S.
Elsworth, Y.
Huber, D.
Hale, S. J.
Houdek, G.
Karoff, C.
Lundkvist, M.
Metcalfe, T. S. [1 ]
Molenda-Zakowicz, J.
Monteiro, M. J. P. F. G.
Thompson, M. J. [1 ]
Stello, D.
Christensen-Dalsgaard, J. [1 ]
Gilliland, R. L.
Kawaler, S. D.
Kjeldsen, H.
Clarke, B. D.
Girouard, F. R.
Hall, J. R.
Quintana, E. V.
Sanderfer, D. T.
Seader, S. E.
机构：
[1] NCAR, High Altitude Observ, Boulder, CO 80307 USA
来源：
PROGRESS IN SOLAR/STELLAR PHYSICS WITH HELIO- AND ASTEROSEISMOLOGY | 2012年 / 462卷
关键词：
SUN-LIKE STAR; ASTEROSEISMOLOGY; OSCILLATIONS; MISSION;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Having started science operations in May 2009, the Kepler photometer has been able to provide exquisite data for solar-like stars. Five out of the 42 stars observed continuously during the survey phase show evidence of oscillations, even though they are rather faint (magnitudes from 10.5 to 12). In this paper, we present an overview of the results of the seismic analysis of 4 of these stars observed during more than eight months.
引用
收藏
页码：180 / 183
页数：4
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