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Simulations of stellar convection, pulsation and semiconvection

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.

preprint2010arXivOpen access
Herbert J. MuthsamFriedrich KupkaEva MundprechtFlorian ZaussingerHannes Grimm-StreleNatalie Happenhofer
astro-ph.SR
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Open access6 authors1 topic
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Herbert J. MuthsamFriedrich KupkaEva MundprechtFlorian ZaussingerHannes Grimm-StreleNatalie Happenhofer

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