Solar-like oscillations in red giants observed with Kepler: comparison of global oscillation parameters from different methods
Context. The large number of stars for which uninterrupted high-precision photometric timeseries data are being collected with Kepler and CoRoT initiated the development of automated methods to analyse the stochastically excited oscillations in main-sequence, subgiant and red-giant stars. Aims: We investigate the differences in results for global
Hekker, S. et al.
Fecha de publicación:
1
2011