Modelling Stellar Convection and Pulsation in Multidimensions Using the ANTARES Code

Chapter
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 31)

Abstract

The ANTARES code has been designed for simulation of astrophysical flows in a variety of situations, in particular in the context of stellar physics. Here, we describe extensions as necessary to model the interaction of pulsation and convection in classical pulsating stars. These extensions comprise the introduction of a spherical grid, moveable in the radial direction, specific forms of grid-refinement and considerations regarding radiative transfer. We then present the basic parameters of the Cepheid we study more closely. For that star we provide a short discussion of patterns of the \(\mbox{ H} + \mbox{ HeI}\) and the \(\mbox{ HeII}\) convection zones and the interaction with pulsation seen in the pdV work or atmospheric structures.

Keywords

Convection Zone Convection Cell Diffusion Approximation Radiative Transfer Equation Ionization Front 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgements

We acknowledge support by the Austrian Science Foundation (P20973).

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Copyright information

© Springer-Verlag Berlin Heidelberg 2013

Authors and Affiliations

  1. 1.Faculty of MathematicsUniversity of ViennaViennaAustria

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