The emergence of spherical magneto-gas dynamic strong shock with radiation near the surface of a star with a rotating, gravitating, non-uniform atmosphere (Q988492)
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scientific article; zbMATH DE number 5775421
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | The emergence of spherical magneto-gas dynamic strong shock with radiation near the surface of a star with a rotating, gravitating, non-uniform atmosphere |
scientific article; zbMATH DE number 5775421 |
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The emergence of spherical magneto-gas dynamic strong shock with radiation near the surface of a star with a rotating, gravitating, non-uniform atmosphere (English)
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27 August 2010
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Summary: 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 is observed that gravitation and rotation have an important impact upon the emergence of shock at the surface of the star.
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spherical magneto-gas dynamic shock wave
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gravitation
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rotation
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