Solution of the flow of self-gravitating gas behind shock wave with radiative flux.

Details Solution of the flow of self-gravitating gas behind shock wave with radiative flux. Solution of the flow of self-gravitating gas behind shock wave with radiative flux.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997injtp..45..169s&link_type=abstract

Indian J. Theor. Phys., Vol. 45, No. 2, p. 169 - 176

Physics

Shock Waves: Propagation

Scientific paper

A solution of the flow variables behind a shock wave propagating into a
self-gravitating gas allowing for the effect of radiative flux using the
Chester-Chisnell-Whitham method has been studied.

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