The terrain of evolution of isotropic adiabatic supernova remnants

Details The terrain of evolution of isotropic adiabatic supernova remnants The terrain of evolution of isotropic adiabatic supernova remnants

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...304..771c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 304, May 15, 1986, p. 771-779.

Astronomy and Astrophysics

Astrophysics

6

Stellar Evolution, Stellar Models, Supernova Remnants, Adiabatic Conditions, Interstellar Gas, Isotropic Media, Magellanic Clouds, Milky Way Galaxy

Scientific paper

Models of the evolution of supernova remnants in isotropic media are reviewed and generalized. It is shown that properties of remnants (including cooling and volume-filling aspects) are almost history-independent functions of their instantaneous average density and postshock temperature. These properties, presented as a contour diagram in the density-temperature plane, thus define the territory through which remnant properties evolve. In different models, remnants merely take different paths across the available terrain. For the Milky Way, M101, and the LMC, the portions of this terrain which might actually be sampled by the remnant populations are discussed briefly.

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