A Monte Carlo simulation of the early spectrum of SN 1993 J

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

By dividing the total energy radiated from the photosphere of a supernovae into a large number of photon packets and then following them in their outward journey, we overcome the problem of line blanketing encountered in usual simulation work. With supporting programs providing the density and abundance distributions in the envelope, our software package can be effectively used for a study of the early spectrum of supernovae. We give an application to the observed spectrum of SN 1993J on 1993-04-13.

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