Density, velocity, and temperature profiles for the extended envelope model of type I Supernovae

Details Density, velocity, and temperature profiles for the extended envelope model of type I Supernovae Density, velocity, and temperature profiles for the extended envelope model of type I Supernovae

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aipc...63....1l&link_type=abstract

AIP Conference Proceedings, Volume 63, pp. 1-3 (1980).

Statistics

Computation

6

Supernovae, Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers

Scientific paper

The early light curve of Type I Supernova has been fitted by a model in which the low density envelope of a supergiant is exploded by the sudden release of energy at its center. This paper supplements previous publications on this model by giving information about the model which is necessary for the computation of the emitted spectrum, namely, the density, temperature and velocity profiles of the expanding shell.

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