Simulations of stellar convection, pulsation and semiconvection
Solar and Stellar Astrophysics
2015-05-19 v1
Abstract
We report on modelling in stellar astrophysics with the ANTARES code. First, we describe properties of turbulence in solar granulation as seen in high-resolution calculations. Then, we turn to the first 2D model of pulsation-convection interaction in a cepheid. We discuss properties of the outer and the HEII ionization zone. Thirdly, we report on our work regarding models of semiconvection in the context of stellar physics.
Keywords
Cite
@article{arxiv.1009.2409,
title = {Simulations of stellar convection, pulsation and semiconvection},
author = {Herbert J. Muthsam and Friedrich Kupka and Eva Mundprecht and Florian Zaussinger and Hannes Grimm-Strele and Natalie Happenhofer},
journal= {arXiv preprint arXiv:1009.2409},
year = {2015}
}
Comments
Astrophysical Dynamics: From Stars to Galaxies. IAU Symposium 271