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Authors: Chaplin, W. J | Appourchaux, T | Brown, T. M | Aguirre, V. S | Stevens, I. R | Suárez, J. C | Suran, M. D | Trampedach, R | Turck-Chièze, S | Uytterhoeven, K | Ventura, R | Wilson, P. A | Christensen-Dalsgaard, J | Gilliland, R. L | Kjeldsen, H | Borucki, W. J | Koch, D | Jenkins, J. M | Ballot, J | Basu, S | Bazot, M | Elsworth, Y | Bedding, T. R | Benomar, O | Bonanno, A | Brandão, I. M | Bruntt, H | Campante, T. L | Creevey, O. L | Mauro, M. P. Di | Doğan, G | Dreizler, S | García, R. A | Eggenberger, P | Esch, L | Fletcher, S. T | Frandsen, S | Gai, N | Gaulme, P | Handberg, R | Hekker, S | Howe, R | Huber, D | Houdek, G | Korzennik, S. G | Lebrun, J. C | Leccia, S | Martic, M | Mathur, S | Mosser, B | New, R | Quirion, P.-O | Régulo, C | Roxburgh, I. W | Karoff, C | Salabert, D | Schou, J | Sousa, S. G | Stello, D | Verner, G. A | Arentoft, T | Barban, C | Belkacem, K | Benatti, S | Biazzo, K | Metcalfe, T. S | Boumier, P | Bradley, P. A | Broomhall, A.-M | Buzasi, D. L | Claudi, R. U | Cunha, M. S | D'Antona, F | Deheuvels, S | Derekas, A | Hernández, A. García | Molenda-Żakowicz, J | Giampapa, M. S | Goupil, M. J | Gruberbauer, M | Guzik, J. A | Hale, S. J | Ireland, M. J | Kiss, L. L | Kitiashvili, I. N | Kolenberg, K | Korhonen, H | Monteiro, M. J. P. F. G | Kosovichev, A. G | Kupka, F | Lebreton, Y | Leroy, B | Ludwig, H.-G | Mathis, S | Michel, E | Miglio, A | Montalbán, J | Moya, A | Thompson, M. J | Noels, A | Noyes, R. W | Pallé, P. L | Piau, L | Preston, H. L | Cortés, T. Roca | Roth, M | Sato, K. H | Schmitt, J | Serenelli, A. M
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137906
Description: We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-nois ... More
Reviewed: Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/139375
Description: The growing interest in solar twins is motivated by the possibility of comparing them directly to the Sun. To carry on this kind of analysis, we need to know their physical characteristics with precis ... More
Full Text: Full Text
Reviewed: Reviewed
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