Three-dimensional adiabatic supernova remnants

Details Three-dimensional adiabatic supernova remnants Three-dimensional adiabatic supernova remnants

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..749b&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, July-Aug. 1991, p. 749-758. In Russian.

Astronomy and Astrophysics

Astronomy

11

Adiabatic Conditions, Hydrodynamic Equations, Stellar Evolution, Supernova Remnants, Three Dimensional Bodies, Density Distribution, Detonation Waves, Equations Of Motion, Gas Density, Wave Propagation

Scientific paper

A numerical hydrodynamic scheme is proposed for calculating the evolution of 3D adiabatic SN remnants in media with an arbitrary density distribution. Consideration is given to the widening in a homogeneous medium of a remnant which is a triaxial ellipsoid at the initial moment, as well as to the evolution of an initially spherically symmetrical blast wave in a medium with an 'ellipsoidal' gas density distribution.

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