The Evolution of Supernovae in the Winds of Massive Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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7 pages, 6 figures, to be published in Cosmic Explosions in Three Dimensions: Asymmetries in Supernovae and Gamma-Ray Bursts,

Scientific paper

We study the evolution of supernova remnants in the circumstellar medium
formed by mass loss from the progenitor star. The properties of this
interaction are investigated, and the specific case of a 35 $\msun$ star is
studied in detail. The evolution of the SN shock wave in this case may have a
bearing on other SNRs evolving in wind-blown bubbles, especially SN 1987A.

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