Physics
Scientific paper
Jan 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006coast.147...61d&link_type=abstract
Communications in Asteroseismology, vol. 147, p. 61-64
Physics
Scientific paper
The problem of the interaction between convection and pulsations is considered. A precise modeling of this interaction is required for the seismic study of stars with non-negligible convective envelope. After a short introduction to the Time-Dependent Convection theory of Gabriel (1996) and Grigahcene et al. (2005), we give a summary of the main results obtained with this treatment for delta Sct, gamma Dor and solar-like stars.
Dupret Marc-Antoine
Gabriel Michael
Garrido Rafa
Grigahcène A.
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