Physical properties of the supernova remnant expanding in a clumpy circumstellar medium.

Details Physical properties of the supernova remnant expanding in a clumpy circumstellar medium. Physical properties of the supernova remnant expanding in a clumpy circumstellar medium.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996sccha..39..197y&link_type=abstract

Science in China, Series A, Vol. 39, No. 2, p. 197 - 206

Physics

Supernova Remnants: Expansion, Supernova Remnants: Circumstellar Matter

Scientific paper

Physical properties of the supernova remnant expanding in a clumpy circumstellar medium are studied. Taking into account the effect of cloud evaporation in the clumpy medium, it is found that the evolution and internal structure of the supernova remnant in a clumpy medium of a power-law density distribution in the radius are generally self-similar as long as the minus power-law index is in the range of about 0 - 3.

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