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Numerical Simulations of 3D Compressible Convection

Published online by Cambridge University Press:  12 April 2016

Herbert J. Muthsam  and
Johann Zöchling
Herbert J. Muthsam
Affiliation:
Institute of MathematicsUniversity of ViennaBoltzmanngasse 5 A–1090 Vienna/Austria e-mail:[email protected]
Johann Zöchling
Affiliation:
Institute of MathematicsUniversity of ViennaBoltzmanngasse 5 A–1090 Vienna/Austria e-mail:[email protected]

Abstract

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Numerical models of a convection zone embedded between two stable layers have been calculated; one is shortly presented and in particular a few items concerning the lower overshoot region are discussed.

Type
III. Input physics for stellar structure
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 296 - 299
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Cattaneo, F. et al. 1991, Ap. J., 370., 282.CrossRefGoogle Scholar
Chan, K.L. and Sofia, S. 1989, Ap. J., 336, 1022.CrossRefGoogle Scholar
Fox, P.A., Theobald, M.L. and Sofia, S. 1991, Ap. J., 383, 860.CrossRefGoogle Scholar
Hossain, M. and Mullan, D.J., 1991, Ap. J., 380, 631.CrossRefGoogle Scholar
Hurlburt, N.E. et al. 1986, Ap. J., 311, 563.CrossRefGoogle Scholar
Lafon, F. and Osher, S. 1991, Journal of Computational Physics, 96, 110.CrossRefGoogle Scholar
Muthsam, H. 1992, in preparation.Google Scholar