Seismic analysis of four solar-like stars observed during more than eight months by Kepler

S. Mathur, T. L. Campante, R. Handberg, R. A. Garcia, T. Appourchaux, T. R. Bedding, B. Mosser, W. J. Chaplin, J. Ballot, O. Benomar, A. Bonanno, E. Corsaro, P. Gaulme, S. Hekker, C. Regulo, D. Salabert, G. Verner, T. R. White, I. M. Brandao, O. L. CreeveyG. Dogan, M. Bazot, M. S. Cunha, Y. Elsworth, D. Huber, S. J. Hale, G. Houdek, C. Karoff, M. Lundkvist, T. S. Metcalfe, J. Molenda-Zakowicz, M. J. P. F. G. Monteiro, M. J. Thompson, D. Stello, J. Christensen-Dalsgaard, R. L. Gilliland, S. D. Kawaler, H. Kjeldsen, B. D. Clarke, F. R. Girouard, J. R. Hall, E. V. Quintana, D. T. Sanderfer, S. E. Seader

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Abstract

Having started science operations in May 2009, the Kepler photometer has been able to provide exquisite data of 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.
OriginalsprogEngelsk
TidsskriftAstronomical Society of the Pacific. Conference Proceedings
ISSN1050-3390
StatusUdgivet - 1 okt. 2011

Emneord

  • astro-ph.SR

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