Oscillation mode frequencies of 61 main-sequence and subgiant stars observed by Kepler
Context. Solar-like oscillations have been observed by Kepler and CoRoT in several solar-type stars, thereby providing a way to probe the stars using asteroseismology Aims: We provide the mode frequencies of the oscillations of various stars required to perform a comparison with those obtained from stellar modelling. Methods: We used a time series
Appourchaux, T. et al.
Fecha de publicación:
7
2012