Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5005
Title: The asteroseismic potential of Kepler: first results for solar-type stars
Authors: Chaplin, W. J
Appourchaux, T
Elsworth, Y
Garcia, R. A
Houdek, G
Karoff, C
Metcalfe, T. S
Molenda-Zakowicz, J
Monteiro, M. J. P. F. G
Thompson, M. J
Brown, T. M
Kiss, L. L
Kitiashvili, I. N
Kolenberg, K
Korhonen, H
Kosovichev, A. G
Kupka, F
Lebreton, Y
Leroy, B
Ludwig, H. G
Mathis, S
Michel, E
Miglio, A
Montalban, J
Moya, A
Noels, A
Noyes, R. W
Palle, P. L
Piau, L
Preston, H. L
Roca Cortes, T
Roth, M
Sato, K. H
Schmitt, J
Serenelli, A. M
Silva Aguirre, V
Stevens, I. R
Suarez, J. C
Suran, M. D
Trampedach, R
Turck-Chieze, S
Uytterhoeven, K
Ventura, R
Christensen-Dalsgaard, J
Gilliland, R. L
Kjeldsen, H
Borucki, W. J
Koch, D
Jenkins, J. M
Ballot, J
Basu, S
Bazot, M
Bedding, T. R
Benomar, O
Bonanno, A
Brandao, I. M
Bruntt, H
Campante, T. L
Creevey, O. L
Di Mauro, M. P
Dogan, G
Dreizler, S
Eggenberger, P
Esch, L
Fletcher, S. T
Frandsen, S
Gai, N
Gaulme, P
Handberg, R
Hekker, S
Howe, R
Huber, D
Korzennik, S. G
Lebrun, J. C
Leccia, S
Martic, M
Mathur, S
Mosser, B
New, R
Quirion, P. O
Regulo, C
Roxburgh, I. W
Salabert, D
Schou, J
Sousa, S. G
Stello, D
Verner, G. A
Arentoft, T
Barban, C
Belkacem, K
Benatti, S
Biazzo, K
Boumier, P
Bradley, P. A
Broomhall, A. M
Buzasi, D. L
Claudi, R. U
Cunha, M. S
D'Antona, F
Deheuvels, S
Derekas, A
Garcia Hernandez, A
Giampapa, M. S
Goupil, M. J
Gruberbauer, M
Guzik, J. A
Hale, S. J
Ireland, M. J
Keywords: Stars: Oscillations;Stars: Interiors;Stars: Late-Type
Issue Date: Apr-2010
Publisher: IOP Publishing
Citation: The Astrophysical Journal, Vol. 713, No. 2, pp. L169 - L175
Abstract: We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5d of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: About 20 modes of oscillation may be clearly distinguished in each star. We discuss the appearance of the oscillation spectra, use the frequencies and frequency separations to provide first results on the radii, masses and ages of the stars, and comment in the light of these results on prospects for inference on other solar-type stars that Kepler will observe.
URI: http://hdl.handle.net/2248/5005
ISSN: 0004-637X
???metadata.dc.rights???: © Institute of Physics
???metadata.dc.relation.uri???: http://arxiv.org/abs/1001.0506
http://iopscience.iop.org/2041-8205/713/2/L169/
Appears in Collections:IIAP Publications

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