Seismic analysis of four solar-like stars observed during more than eight months by Kepler
| Authors |
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| Publication date | 2012 |
| Host editors |
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| Book title | Progress in Solar/Stellar Physics with Helio- and Asteroseismology |
| Book subtitle | proceedings of a Fujihara Seminar held at Hakone, Japan, in 13-17 March 2011 |
| ISBN |
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| ISBN (electronic) |
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| Series | Astronomical Society of the Pacific conference series |
| Event | 61st Fujihara Seminar “Progress in Solar / Stellar Physics with Helio- and Asteroseismology” |
| Pages (from-to) | 180-183 |
| Publisher | San Francisco: Astronomical Society of the Pacific |
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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. |
| Document type | Conference contribution |
| Language | English |
| Published at | http://aspbooks.org/a/volumes/article_details/?paper_id=34563 |
| Other links | http://adsabs.harvard.edu/abs/2012ASPC..462..180M |
| Downloads |
1110.0135v1.pdf
(Accepted author manuscript)
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