Non-adiabatic study of the Kepler subgiant KIC 6442183

Thanks to the precision of Kepler observations, [3] were able to measure the linewidth and amplitude of individual modes (including mixed modes) in several subgiant power spectra. We perform a forward modelling of a Kepler subgiant based on surface properties and observed frequencies. Non-adiabatic...

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Bibliographic Details
Main Authors: Grosjean M., Dupret M.A., Belkacem K., Benomar O., Deheuvels S., Samadi R., Grigahcene A.
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201510106028