A study of stellar point explosion in a self-gravitating radiative magneto-hydrodynamic medium

Details A study of stellar point explosion in a self-gravitating radiative magneto-hydrodynamic medium A study of stellar point explosion in a self-gravitating radiative magneto-hydrodynamic medium

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.183..135n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 183, no. 1, Sept. 1991, p. 135-145.

Statistics

Computation

2

Gravitational Effects, Magnetohydrodynamics, Shock Wave Propagation, Stellar Physics, Boundary Conditions, Computational Astrophysics, Differential Equations, Interstellar Magnetic Fields, Runge-Kutta Method

Scientific paper

A theoretical model of shock wave propagation in a self-gravitating
radiative magnetohydrodynamic medium has been studied. The effects of
the magnetic field, radiation, and gravitation have been discussed
separately. The results discussed depend upon the numerical variations
of flow variables behind the shock.

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