- Seismic analysis of four solar-like stars observed during more than eight months by Kepler
- Astronomical Society of the Pacific conference series
- Pages (from-to)
- Document type
- Faculty of Science (FNWI)
- Anton Pannekoek Institute for Astronomy (API)
- 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.
Proceedings title: Progress in solar/stellar physics with helio- and asteroseismology: proceedings of a Fujihara Seminar held at Hakone, Japan, in 13-17 March 2011
Publisher: Astronomical Society of the Pacific
Place of publication: San Francisco
Editors: H. Shibahashi, M. Takata, A.E. Lynas-Gray
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