Construction of analytical light curves of SN 1987A, taking the cooling and recombination wave into account

Details Construction of analytical light curves of SN 1987A, taking the cooling and recombination wave into account Construction of analytical light curves of SN 1987A, taking the cooling and recombination wave into account

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..497i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 3, May-June 1992, p. 497-515. In Russian.

Statistics

Computation

11

Computational Astrophysics, Cooling Flows (Astrophysics), Light Curve, Recombination Reactions, Stellar Models, Supernova 1987A, Differential Equations, Radioactive Isotopes, Stellar Temperature

Scientific paper

Analytical models of supernovae which make it possible to reduce the problem of calculating the bolometric light curves to the solution of ordinary differential equations are examined. These models consistently take into account the cooling and recombination wave (CRW). It is shown that a rather good agreement between the analytical models and observations of SN 1987A after about 40 days can be obtained only if the WCR is taken into account.

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