RESEARCH
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Asteroseismology of solar-type stars with Kepler: II. Stellar modeling

T. S. Metcalfe, M. J. P. F. G. Monteiro, M. J. Thompson, W. J. Chaplin, S. Basu, A. Bonanno, M. P. Di Mauro, G. Doǧan, P. Eggenberger, C. Karoff, D. Stello, KASC WG1

Abstract
Observations from the Kepler satellite were recently published for three bright G-type stars, which were monitored during the first 33.5 d of science operations. One of these stars, KIC 11026764, exhibits a characteristic pattern of oscillation frequencies suggesting that the star has evolved significantly. We have derived initial estimates of the properties of KIC 11026764 from the oscillation frequencies observed by Kepler, combined with ground-based spectroscopic data. We present preliminary results from detailed modeling of this star, employing a variety of independent codes and analyses that attempt to match the asteroseismic and spectroscopic constraints simultaneously.

Keywords
stars: individual (KIC 11026764) - stars: interiors - stars:late-type - stars: oscillations

Notes
The Kepler Asteroseismic Science Consortium Working Group 1 also includes: Appourchaux, T., Elsworth, Y., Garcia, R.A., Houdek, G., Molenda-Żakowicz, J., Brown, T.M., Christensen-Dalsgaard, J., Gilliland, R.L., Kjeldsen, H., Borucki,W.J.,Koch, D., Jenkins, J.M., Ballot, J., Bazot, M., Bedding, T.R., Benomar, O., Brandao, I.M., Bruntt, H., Campante, T.L., Creevey, O.L., Dreizler, S., 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., 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., 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 & Wilson, P.A.

Astronomische Nachrichten
Volume 331, Number 9-10, Page 977
2010 December

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Instituto de Astrofísica e Ciências do Espaço Universidade do Porto Faculdade de Ciências da Universidade de Lisboa
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia