1 Result Found

Advanced Search

Select all

Results per page

Select all

Article

1,418 Views

11 Pages

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

Ashok Ganguly and
Pankaj Sharma

Math. Comput. Appl.2010, 15(3), 461-471;https://doi.org/10.3390/mca15030461

-

1 December 2010

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 rat...

Full Article