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Simulations of stellar convection, pulsation and semiconvection

Published online by Cambridge University Press:  12 August 2011

Herbert J. Muthsam
Affiliation:
Faculty of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: herbert.muthsam@univie.ac.at
Friedrich Kupka
Affiliation:
Faculty of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: herbert.muthsam@univie.ac.at
Eva Mundprecht
Affiliation:
Faculty of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: herbert.muthsam@univie.ac.at
Florian Zaussinger
Affiliation:
Faculty of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: herbert.muthsam@univie.ac.at Max Planck Institute for Astrophysics, Karl Schwarzschildstrasse 1, D-85741 Garching, Germany
Hannes Grimm-Strele
Affiliation:
Faculty of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: herbert.muthsam@univie.ac.at
Natalie Happenhofer
Affiliation:
Faculty of Mathematics, University of Vienna, Nordbergstrasse 15, A-1090 Vienna, Austria email: herbert.muthsam@univie.ac.at
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Abstract

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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

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