Seismic Analysis of Four Solar-like Stars Observed during More Than Eight Months by Kepler

• Type: Article in International Conference Proceedings Book
• Date: 2012

Authors

Mathur, S (Author) Other; Campante, TL (Author) Other; Handberg, R (Author) Other; Garcia, RA (Author) Other; Appourchaux, T (Author) Other; Bedding, TR (Author) Other; Mosser, B (Author) Other; Chaplin, WJ (Author) Other; Ballot, J (Author) Other; Benomar, O (Author) Other; Bonanno, A (Author) Other; Corsaro, E (Author) Other; Gaulme, P (Author) Other; Hekker, S (Author) Other; Regulo, C (Author) Other; Salabert, D (Author) Other; Verner, G (Author) Other; White, TR (Author) Other; Brandao, IM (Author) Other; Creevey, OL (Author) Other; Dogan, G (Author) Other; Bazot, M (Author) Other; Cunha, MS (Author) FCUP; Elsworth, Y (Author) Other; Huber, D (Author) Other; Hale, SJ (Author) Other; Houdek, G (Author) Other; Karoff, C (Author) Other; Lundkvist, M (Author) Other; Metcalfe, TS (Author) Other; Molenda Zakowicz, J (Author) Other; Monteiro, MJPFG (Author) FCUP; Thompson, MJ (Author) Other; Stello, D (Author) Other; Christensen Dalsgaard, J (Author) Other; Gilliland, RL (Author) Other; Kawaler, SD (Author) Other; Kjeldsen, H (Author) Other; Clarke, BD (Author) Other; Girouard, FR (Author) Other; Hall, JR (Author) Other; Quintana, EV (Author) Other; Sanderfer, DT (Author) Other; Seader, SE (Author) Other

Conference proceedings International

Title: PROGRESS IN SOLAR/STELLAR PHYSICS WITH HELIO- AND ASTEROSEISMOLOGY

Pages: 180-183

61st Fujihara Seminar on Helio- and Asterseismology

Hakone, JAPAN, MAR 13-17, 2011

Indexing

ISI Web of Knowledge - 0 Citations

Scientific classification

FOS: Natural sciences > Physical sciences

CORDIS: Physical sciences > Astronomy

Other information

Authenticus ID: P-008-KNH

Abstract (EN): Having started science operations in May 2009, the Kepler photometer has been able to provide exquisite data for 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.

Language: English

Type (Professor's evaluation): Scientific