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Modelling Stellar Convection and Pulsation in Multidimensions Using the ANTARES Code

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Stellar Pulsations

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

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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.

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References

  1. Buchler, J.R.: In: Ferlet, R., Maillard, J.P., Raban, B. (eds.) Variables Stars and the Astrophysical Returns of the Microlensing Surveys, p. 181 (1997)

    Google Scholar 

  2. Buchler, J.R.: In: American Institute of Physics Conference Series, vol. 1170, 51 (2009)

    Google Scholar 

  3. Carlson, B.G.: In: Alder, B., Fernbach, S. (eds.) Methods in Computational Physics, vol. 1 (1963)

    Google Scholar 

  4. Kunasz, P., Auer, L.H.: JQSRT 39, 67 (1988)

    Article  ADS  Google Scholar 

  5. Muthsam, H.J., Kupka, F., Löw-Baselli, B., et al: NewAst 15, 460 (2010)

    Article  ADS  Google Scholar 

  6. Spiegel, E.A.: ApJ 126, 202 (1957)

    Article  MathSciNet  ADS  Google Scholar 

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Acknowledgements

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

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Correspondence to Eva Mundprecht .

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Mundprecht, E., Muthsam, H.J. (2013). Modelling Stellar Convection and Pulsation in Multidimensions Using the ANTARES Code. In: Suárez, J., Garrido, R., Balona, L., Christensen-Dalsgaard, J. (eds) Stellar Pulsations. Astrophysics and Space Science Proceedings, vol 31. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-29630-7_10

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  • DOI: https://doi.org/10.1007/978-3-642-29630-7_10

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