Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..90..153s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 90, no. 1, Feb. 1983, p. 153-159.
Astronomy and Astrophysics
Astrophysics
3
Gas Flow, Nonuniform Flow, Radiative Heat Transfer, Shock Wave Propagation, Spherical Waves, Stellar Atmospheres, Density Distribution, Flow Equations, Gray Gas, Mass Distribution, Pressure Distribution, Radiation Distribution, Similarity Numbers, Velocity Distribution
Scientific paper
Self-similar flows of self-gravitating gas behind the spherical shock wave propagating in a nonuniform atmosphere at rest are investigated, taking radiation heat flux into consideration. The radiation pressure and radiation energy are neglected, and the gas is assumed to be gray, opaque, and at rest in the undisturbed field. The shock is assumed to be transparent and isothermal, and the total energy of the explosion is assumed to be nonconstant and varying with time. The equations of motion and boundary conditions are analyzed, and solutions for the differential equation are presented. Distributions of the velocity, density, mass, pressure, and radiation flux for the flow are shown.
Vishwakarma P. R.
~Singh ~B. J.
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