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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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.
Original languageEnglish
JournalAstronomical Society of the Pacific. Conference Proceedings
Publication statusPublished - 1 Oct 2011

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