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

@article{Chaplin2010TheAP,
  title={The Asteroseismic potential of Kepler : first results for solar-type stars},
  author={W. Chaplin and T. Appourchaux and Y. Elsworth and R. Garc{\'i}a and G. Houdek and C. Karoff and T. Metcalfe and J. Molenda-.Zakowicz and M. Monteiro and M. Thompson and T. Brown and J. Christensen-Dalsgaard and R. Gilliland and H. Kjeldsen and W. Borucki and D. Koch and J. Jenkins and J. Ballot and S. Basu and M. Bazot and T. Bedding and O. Benomar and A. Bonanno and I. Brand{\~a}o and H. Bruntt and T. Campante and O. Creevey and M. D. Mauro and G. Dogan and S. Dreizler and P. Eggenberger and L. Esch and S. Fletcher and S. Frandsen and N. Gai and P. Gaulme and R. Handberg and S. Hekker and R. Howe and D. Huber and S. Korzennik and J. Lebrun and S. Leccia and M. Marti{\'c} and S. Mathur and B. Mosser and R. New and P.-O. Quirion and C. R'egulo and I. Roxburgh and D. Salabert and J. Schou and S. Sousa and D. Stello and G. Verner and T. Arentoft and C. Barban and K. Belkacem and S. Benatti and K. Biazzo and P. Boumier and P. Bradley and A.-M. Broomhall and D. Buzasi and R. Claudi and M. Cunha and F. D'antona and S. Deheuvels and A. Derekas and A. Hern'andez and M. Giampapa and M. J. Goupil and M. Gruberbauer and J. Guzik and S. Hale and M. Ireland and L. Kiss and I. Kitiashvili and K. Kolenberg and H. Korhonen and A. Kosovichev and F. Kupka and Y. Lebreton and B. LeRoy and H. Ludwig and S. Mathis and E. Michel and A. Miglio and J. Montalb'an and A. Moya and A. Noels and R. Noyes and P. Pall'e and L. Piau and H. Preston and T. Cort{\'e}s and M. Roth and K. Sato and J. Schmitt and A. Serenelli and V. Aguirre and I. Stevens and J. C. Su{\'a}rez and M. Suran and R. Trampedach and S. Turck-chi{\`e}ze and K. Uytterhoeven and R. Ventura},
  journal={The Astrophysical Journal},
  year={2010},
  volume={713}
}
  • W. Chaplin, T. Appourchaux, +105 authors R. Ventura
  • Published 2010
  • Physics
  • The Astrophysical Journal
  • 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… CONTINUE READING
    118 Citations

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