Late-stage evolution of supernova remnants

Details Late-stage evolution of supernova remnants Late-stage evolution of supernova remnants

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979phdt.........4n&link_type=abstract

Ph.D. Thesis Cornell Univ., Ithaca, NY.

Mathematics

1

Stellar Evolution, Supernova Remnants, Supernovae, Interstellar Space, Mathematical Models, Stellar Models, Thermal Instability

Scientific paper

The evolution of spherically symmetric supernova remnants is examined by analytic and numerical means. The blast is assumed to take place in an homogeneous interstellar medium with a uniform density and an initially constant total energy. An approximate representation of the radiative cooling is included, precipitating a thermal instability and producing a cold dense shell. The dynamical transition from adiabatic to radiation dominated behavior is numerically simulated by a modified form of the pseudo viscosity method.

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