Implicit hydrodynamic simulations of stellar interiors
classification
🌌 astro-ph.SR
astro-ph.IM
keywords
stellarcodefirsthydrodynamicimplicitconvectiondevelopmentevolution
read the original abstract
We report on the development of an implicit multi-D hydrodynamic code for stellar evolution. We present two test-cases relevant for the first scientific goal of the code: the simulation of convection in pulsating stars. First results on a realistic stellar model are also presented.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.