RADIUS DETERMINATION OF SOLAR-TYPE STARS USING ASTEROSEISMOLOGY: WHAT TO EXPECT FROM THE KEPLER MISSION
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T. Appourchaux | J. Christensen-Dalsgaard | S. G. Sousa | D. Stello | O. L. Creevey | T. R. Bedding | T. Arentoft | H. Kjeldsen | T. Toutain | H. Bruntt | P.-O. Quirion | P. Quirion | T. Bedding | S. Sousa | H. Kjeldsen | J. Christensen-Dalsgaard | W. Chaplin | D. Stello | A. Moya | J. Ballot | O. Creevey | H. Bruntt | T. Arentoft | S. Fletcher | R. New | T. Appourchaux | R. García | W. J. Chaplin | A. Garc'ia-Hern'andez | M. J. P. F. G. Monteiro | A. Moya | J.-C. Su'arez | J. Ballot | Y. Elsworth | S. T. Fletcher | R. A. Garc'ia | Gunter Houdek | S. J. Jim'enez-Reyes | R. New | C. R'egulo | D. Salabert | G. Houdek | J. Suárez | M. Monteiro | Y. Elsworth | T. Toutain | D. Salabert | C. Régulo | S. Jiménez-Reyes | Antonio García-Hernández
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