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Article

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

by
Ashok Ganguly
1 and
Pankaj Sharma
2,*
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
Published: 1 December 2010
Versions Notes

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.
Keywords: Spherical Magneto-gas dynamic shock wave; Gravitation; Rotation Spherical Magneto-gas dynamic shock wave; Gravitation; Rotation

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MDPI and ACS Style

Ganguly, A.; Sharma, P. The Emergence of Spherical Magneto-Gas Dynamic Strong Shock with Radiation near the Surface of a Star with a Rotating , Gravitating, Non-Uniform Atmosphere. Math. Comput. Appl. 2010, 15, 461-471. https://doi.org/10.3390/mca15030461

AMA Style

Ganguly A, Sharma P. The Emergence of Spherical Magneto-Gas Dynamic Strong Shock with Radiation near the Surface of a Star with a Rotating , Gravitating, Non-Uniform Atmosphere. Mathematical and Computational Applications. 2010; 15(3):461-471. https://doi.org/10.3390/mca15030461

Chicago/Turabian Style

Ganguly, Ashok, and Pankaj Sharma. 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" Mathematical and Computational Applications 15, no. 3: 461-471. https://doi.org/10.3390/mca15030461

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