A self-similar flow of self-gravitating gas behind a shock wave with increasing energy. I

Details A self-similar flow of self-gravitating gas behind a shock wave with increasing energy. I A self-similar flow of self-gravitating gas behind a shock wave with increasing energy. I

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..87..347s&link_type=abstract

Astrophysics and Space Science, vol. 87, no. 1-2, Oct. 1982, p. 347-355.

Astronomy and Astrophysics

Astrophysics

4

Adiabatic Flow, Gas Flow, Shock Wave Profiles, Shock Wave Propagation, Stellar Mass Ejection, Astrophysics, Equations Of Motion, Isothermal Flow, Mass Distribution, Pressure Distribution, Shock Fronts, Time Dependence, Velocity Distribution

Scientific paper

Self-similar flows of a self-gravitating gas behind a spherical shock wave which are driven out by a propelling contact surface, propagating in a nonuniform atmosphere at rest, are investigated. The total energy content of the flow between the shock front and the contact surface is taken to be time-dependent. In brief, the self-similar homothermal flows of a self-gravitating gas behind a shock wave and Roche's model case are also studied in the present paper.

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