2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/13689We review recent results of stellar pulsation modelling that show that even very simple one-dimensional models for time dependent turbulent energy diffusion and convection provide a substantial improvement over purely radiative models.Workshop on Stellar Structure: Theory and Tests of Convective Energy Transport, Granada, SPAIN, 1998 (to be published in the ASP Conf. Ser.)Astrophysicstext