Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334..266b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 334, Nov. 1, 1988, p. 266-278.
Astronomy and Astrophysics
Astrophysics
13
Adiabatic Conditions, Nebulae, Supernova Remnants, Astronomical Models, Radio Emission
Scientific paper
The adiabatic expansion of a supernova into the surrounding medium is studied numerically in one dimension. The expansion is followed from the early self-similar phase, when the ejecta envelope expands into the ambient medium, until a blast wave develops. The authors study the expansion of models of Type I and II supernovae into either the interstellar medium (with a constant density) or a dense circumstellar medium (with an r-2 density profile) surrounded by a constant density interstellar medium. It is found that numerical calculations are sensitive to both the spatial zoning and the initial ejecta configuration.
Band David L.
Liang Edison P.
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