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Non-adiabatic pulsational observables of Gamma Dor and Delta Scuti stars: comparison of two different numerical codes
R. Garrido1, M.A. Dupret2, A. Claret1 and
A.Moya1
1 Instituto de Astrofisica de Andalucia, CSIC,
Apartado 3004, E-18080 Granada, Spain
2 Institut d'Astrophysique et de Géophysique de l'Universitè de Liège Bât. B5c. Allée du 6 Août, 17 B-4000 Liège Belgium
We present a theoretical study of the non-adiabatic pulsational
observables of Gamma Dor and Delta Scuti stars. We focus our study on the
phase lag
Last changed: 2002/Jun/21
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