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

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

2011-10-01

arxiv.org/abs/1110.0135v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

5 pages, 1 figure. To appear in the ASP proceedings of "The 61st Fujihara seminar: Progress in solar/stellar physics with heli

Scientific paper

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.

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