
doi: 10.1007/bf00656450
The Brinkley-Kirkwood theory, as modified by Bhatnagar and Kushwaha for the inclusion of radiation pressure, is applied to obtain an exact analytical solution for radiation pressure, shock velocity, etc., when a strong explosion takes place in a cold undisturbed gas obeying an exponential density distribution. Cases involving spherical symmetry, axial symmetry or spheroidal symmetry are also considered.
strong explosion, Radiative transfer in astronomy and astrophysics, gas pressure, Gas dynamics (general theory), radiation pressure, Brinkley-Kirkwood theory, exact analytical solutions
strong explosion, Radiative transfer in astronomy and astrophysics, gas pressure, Gas dynamics (general theory), radiation pressure, Brinkley-Kirkwood theory, exact analytical solutions
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