|
|
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
©1996-2002 CAUP |
and other non-adiabatic parameters. These
observables were obtained taking into account interaction with the
atmosphere and neglecting convection. Results from two different equilibrium
and pulsation codes, as developped in Liege and Granada, are compared.