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Chaplin William J., Appourchaux Thierry, Elsworth Yvonne P., Garcia Rafael A., Houdek Günter, Karoff Christoffer, Metcalfe Travis S., Molenda-Zakowicz Joanna, Monteiro M. J. P. F. G., Thompson Michael J., Brown Timothy M., Christensen-Dalsgaard Jörgen, Gilliland Ronald L., Kjeldsen Hans, Borucki William J., Koch David, Jenkins Jon M., Ballot Jérôme, Basu Sarbani, Bazot Michaël, Bedding Timothy R., Benomar Othman, Bonanno Alfio, Brandão I. M., Bruntt H., Campante Tiago L., Creevey Orlagh L., Di Mauro Maria Pia, Dogan Gülnur, Dreizler Stefan, Eggenberger Patrick, Esch Lisa, Fletcher Stephen T., Frandsen Søren, Gai Ning, Gaulme Patrick, Handberg Rasmus, Hekker Saskia, Howe R., Huber Daniel, Korzennik S. G., Lebrun Jean-Claude, Leccia Silvio, Martic Milena, Mathur Savita, Mosser Benoît, New R., Quirion Pierre-Olivier, Regulo Clara, Roxburgh Ian W., Salabert David, Schou Jesper, Sousa S. G., Stello Dennis, Verner Graham A., Arentoft Torben, Barban Caroline, Belkacem Kevin, Benatti Serena, Biazzo Katia, Boumier P., Bradley P. A., Broomhall A. M., Buzasi D. L., Claudi Riccardo U., Cunha M. S., D'Antona Francesca, Deheuvels Sébastien, Derekas A., García Hernández A., Giampapa M. S., Goupil Marie-José, Gruberbauer Michael, Guzik Joyce A., Hale S. J., Ireland Michael J., Kiss László L., Kitiashvili I. N., Kolenberg K., Korhonen H., Kosovichev A. G., Kupka Friedrich, Lebreton Yveline, Leroy A., Ludwig Hans-Günter, Mathis Stéphane, Michel Eric, Miglio Andrea, Montalbán Josefina, Moya Andrés, Noels Arlette, Noyes R. W., Palle P. L., Piau Laurent, Preston H. L., Roca Cortés Teodoro, Roth M., Sato K. H., Schmitt Jérôme, Serenelli Aldo, Aguirre Victor Silva, Stevens Ian R., Suárez Juan Carlos, Suran M. D., Trampedach R., Turck-Chieze Sylvaine, Uytterhoeven K., Ventura R., Wilson P. A.

The Asteroseismic Potential of Kepler: First Results for Solar-Type Stars

The Astrophysical Journal Letters, 2010, vol. 713, pp. L169-L175

Référence DOI : 10.1088/2041-8205/713/2/L169
Référence ADS : 2010ApJ...713L.169C

Résumé :

We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5 days 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.

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