Forms of supernova remnants

Details Forms of supernova remnants Forms of supernova remnants

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..479i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 3, May-June 1992, p. 479-488. In Russian.

Astronomy and Astrophysics

Astronomy

1

Neutron Stars, Stellar Evolution, Stellar Structure, Supernova Remnants, Binary Stars, Interstellar Matter, Stellar Envelopes, Stellar Mass Ejection, Stellar Models, Stellar Winds

Scientific paper

Mechanisms responsible for observed nonsphericity of supernova remnants are analyzed. The following aspects are studied numerically: the influence of the initial homogeneity of the distribution of circumstellar matter on the dynamics of ejecta and the dynamics of SN remnants moving in homogeneous gas. The conclusion is drawn that the factor responsible for observed forms of SN remnants in the adiabatic stage of their evolution is homogeneity of the circumstellar medium.

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