open clusters and associations: individual (NGC 6819); stars: fundamental parameters; stars: interiors; stars: oscillations; techniques: photometric
Abstract :
[en] This article summaries a talk given at the HELAS IV international meeting We present a brief overview of the history of attempts to obtain a clear detection of solar-like oscillations in cluster stars, and discuss the results on the first clear detection, which was made by the Kepler Asteroseismic Science Consortium (KASC) Working Group 2. Data from Kepler.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Stello, D.; Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
Basu, S.; Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA
Bedding, T. R.; Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
Brogaard, K.; Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
Bruntt, H.; LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris, 92195 Meudon, France
Chaplin, W. J.; School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
Christensen-Dalsgaard, J.; Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
Demarque, P.; Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA
Elsworth, Y. P.; School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
