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Strong spherical magnetogasdynamic shock waves in rotating stellar atmosphere

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Abstract

An analytic expression for the velocity of magnetogasdynamic shock wave, propagating in rotating inter stellar atmosphere has been obtained by using the method of characteristics and considering the effect of coriolis force. It has been shown that in the outer convective layer of the star Coriolis force and magnetic field both have significant effect on the shock velocity.

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  1. Department of Mathematics, Gorakhpur University, Gorakhpur, U.P., India

    B. G. Verma, R. C. Srivastava & A. H. Khan

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  1. B. G. Verma
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  2. R. C. Srivastava
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  3. A. H. Khan
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Verma, B.G., Srivastava, R.C. & Khan, A.H. Strong spherical magnetogasdynamic shock waves in rotating stellar atmosphere. Astrophys Space Sci 82, 307–309 (1982). https://doi.org/10.1007/BF00651441

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  • DOI: https://doi.org/10.1007/BF00651441

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