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The asteroseismic potential of Kepler: first results for solar-type stars

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dc.contributor.author Chaplin, W. J
dc.contributor.author Appourchaux, T
dc.contributor.author Elsworth, Y
dc.contributor.author Garcia, R. A
dc.contributor.author Houdek, G
dc.contributor.author Karoff, C
dc.contributor.author Metcalfe, T. S
dc.contributor.author Molenda-Zakowicz, J
dc.contributor.author Monteiro, M. J. P. F. G
dc.contributor.author Thompson, M. J
dc.contributor.author Brown, T. M
dc.contributor.author Kiss, L. L
dc.contributor.author Kitiashvili, I. N
dc.contributor.author Kolenberg, K
dc.contributor.author Korhonen, H
dc.contributor.author Kosovichev, A. G
dc.contributor.author Kupka, F
dc.contributor.author Lebreton, Y
dc.contributor.author Leroy, B
dc.contributor.author Ludwig, H. G
dc.contributor.author Mathis, S
dc.contributor.author Michel, E
dc.contributor.author Miglio, A
dc.contributor.author Montalban, J
dc.contributor.author Moya, A
dc.contributor.author Noels, A
dc.contributor.author Noyes, R. W
dc.contributor.author Palle, P. L
dc.contributor.author Piau, L
dc.contributor.author Preston, H. L
dc.contributor.author Roca Cortes, T
dc.contributor.author Roth, M
dc.contributor.author Sato, K. H
dc.contributor.author Schmitt, J
dc.contributor.author Serenelli, A. M
dc.contributor.author Silva Aguirre, V
dc.contributor.author Stevens, I. R
dc.contributor.author Suarez, J. C
dc.contributor.author Suran, M. D
dc.contributor.author Trampedach, R
dc.contributor.author Turck-Chieze, S
dc.contributor.author Uytterhoeven, K
dc.contributor.author Ventura, R
dc.contributor.author Christensen-Dalsgaard, J
dc.contributor.author Gilliland, R. L
dc.contributor.author Kjeldsen, H
dc.contributor.author Borucki, W. J
dc.contributor.author Koch, D
dc.contributor.author Jenkins, J. M
dc.contributor.author Ballot, J
dc.contributor.author Basu, S
dc.contributor.author Bazot, M
dc.contributor.author Bedding, T. R
dc.contributor.author Benomar, O
dc.contributor.author Bonanno, A
dc.contributor.author Brandao, I. M
dc.contributor.author Bruntt, H
dc.contributor.author Campante, T. L
dc.contributor.author Creevey, O. L
dc.contributor.author Di Mauro, M. P
dc.contributor.author Dogan, G
dc.contributor.author Dreizler, S
dc.contributor.author Eggenberger, P
dc.contributor.author Esch, L
dc.contributor.author Fletcher, S. T
dc.contributor.author Frandsen, S
dc.contributor.author Gai, N
dc.contributor.author Gaulme, P
dc.contributor.author Handberg, R
dc.contributor.author Hekker, S
dc.contributor.author Howe, R
dc.contributor.author Huber, D
dc.contributor.author Korzennik, S. G
dc.contributor.author Lebrun, J. C
dc.contributor.author Leccia, S
dc.contributor.author Martic, M
dc.contributor.author Mathur, S
dc.contributor.author Mosser, B
dc.contributor.author New, R
dc.contributor.author Quirion, P. O
dc.contributor.author Regulo, C
dc.contributor.author Roxburgh, I. W
dc.contributor.author Salabert, D
dc.contributor.author Schou, J
dc.contributor.author Sousa, S. G
dc.contributor.author Stello, D
dc.contributor.author Verner, G. A
dc.contributor.author Arentoft, T
dc.contributor.author Barban, C
dc.contributor.author Belkacem, K
dc.contributor.author Benatti, S
dc.contributor.author Biazzo, K
dc.contributor.author Boumier, P
dc.contributor.author Bradley, P. A
dc.contributor.author Broomhall, A. M
dc.contributor.author Buzasi, D. L
dc.contributor.author Claudi, R. U
dc.contributor.author Cunha, M. S
dc.contributor.author D'Antona, F
dc.contributor.author Deheuvels, S
dc.contributor.author Derekas, A
dc.contributor.author Garcia Hernandez, A
dc.contributor.author Giampapa, M. S
dc.contributor.author Goupil, M. J
dc.contributor.author Gruberbauer, M
dc.contributor.author Guzik, J. A
dc.contributor.author Hale, S. J
dc.contributor.author Ireland, M. J
dc.date.accessioned 2010-02-09T13:38:15Z
dc.date.available 2010-02-09T13:38:15Z
dc.date.issued 2010-04
dc.identifier.citation The Astrophysical Journal, Vol. 713, No. 2, pp. L169 - L175 en
dc.identifier.issn 0004-637X
dc.identifier.uri http://hdl.handle.net/2248/5005
dc.description.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. en
dc.language.iso en en
dc.publisher IOP Publishing en
dc.relation.uri http://arxiv.org/abs/1001.0506 en
dc.relation.uri http://iopscience.iop.org/2041-8205/713/2/L169/
dc.rights © Institute of Physics en
dc.subject Stars: Oscillations en
dc.subject Stars: Interiors en
dc.subject Stars: Late-Type en
dc.title The asteroseismic potential of Kepler: first results for solar-type stars en
dc.type Article en


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