Self-similar model of magnetohydrodynamic radiative shock waves with increasing density

Details Self-similar model of magnetohydrodynamic radiative shock waves with increasing density Self-similar model of magnetohydrodynamic radiative shock waves with increasing density

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.148..143o&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 148, no. 1, Oct. 1988, p. 143-148.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics, Radiant Flux Density, Shock Waves, Gravitational Effects, Magnetic Fields, Perturbation Theory, Radiation Pressure, Star Formation, Supernovae

Scientific paper

The magnetohydrodynamic model of shock waves has been discussed in an
atmosphere with gravitation and radiation. The disturbance is headed by
a strong shock of increasing density. The medium ahead of the shock is
assumed to be inhomogeneous and at rest. Variation of magnetic field,
radiation flux, and other flow variables are given in tabular form.

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