Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146..333n&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 2, July 1988, p. 333-338.
Astronomy and Astrophysics
Astrophysics
Density Distribution, Gravitational Effects, Shock Waves, Magnetohydrodynamic Waves, Perturbation Theory, Runge-Kutta Method, Spherical Waves, Wave Propagation
Scientific paper
Similarity solution for the spherical shock waves propagating in a self-gravitating medium are presented. The medium ahead of the shock is assumed to be inhomogeneous and at rest. The shock radius is assumed to vary with some power of time. The Runga-Kutta method has been used for numerical calculation of the problem. The variations of the flow variables behind the shock have been given in tabular form.
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