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We present a new implementation of the Riccati method for the linear stability analysis of weakly non-adiabatic g-mode pulsations in γ Doradus stars.
Type
Part 4. The Interaction between Convection and Pulsation
Löffler, W.2000, in ASP Conf. Ser., Vol. 203, The impact of Large-Scale Surveys on Pulsating Star Research, eds. Szabados, L. & Kurtz, D., (San Francisco: ASP), 447Google Scholar
Pamyatnykh, A.A.2000, in ASP Conf. Ser., Vol. 210, Delta Scuti and Related Stars, eds. Breger, M. & Montgomery, M., (San Francisco: ASP), 215Google Scholar