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Mathematical and Computational Applications
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  • Mathematical and Computational Applications is published by MDPI from Volume 21 Issue 1 (2016). Previous articles were published by another publisher in Open Access under a CC-BY (or CC-BY-NC-ND) licence, and they are hosted by MDPI on mdpi.com as a courtesy and upon agreement with Association for Scientific Research (ASR).
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1 December 2010

The Emergence of Spherical Magneto-Gas Dynamic Strong Shock with Radiation near the Surface of a Star with a Rotating , Gravitating, Non-Uniform Atmosphere

and
1
Department of Applied Mathematics and Computational Science, 1Shri G. S. Institute of Technology and Science, Indore (M.P.), 452003, India
2
Jawaharlal Institute of Technology, Borawan (Khargone) -451228, India
*
Author to whom correspondence should be addressed.
Math. Comput. Appl.2010, 15(3), 461-471;https://doi.org/10.3390/mca15030461
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Abstract

The propagation of a strong magneto-gas dynamic, rotating and gravitating shock wave originating in a stellar interior is considered, when it approaches the surface of the star. The flow behind the shock wave is assumed to be spatially isothermal rather than adiabatic to simulate the conditions of large radiative transfer near the stellar surface. It has been observed that gravitation and rotation have important impact upon the emergence of shock at the surface of the star.

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