1999/01/14 by J. R. Buchler, J. Robert Buchler, Buchler, J. Robert +7
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9901188
Workshop on Stellar Structure: Theory and Tests of Convective Energy Transport, Granada, SPAIN, 1998 (to be published in the ASP Conf. Ser.)
arxiv created 1999/01/14 · openalex publication_date 1999/01/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We 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.