The Evolution of Supernovae in the Winds of Massive Stars

dc.creatorDwarkadas, Vikram
dc.date2004-03-08
dc.date.accessioned2026-07-07T02:12:33Z
dc.date.available2026-07-07T02:12:33Z
dc.descriptionWe 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.
dc.description7 pages, 6 figures, to be published in Cosmic Explosions in Three Dimensions: Asymmetries in Supernovae and Gamma-Ray Bursts, eds P. Hoeflich, P, Kumar and J. C. Wheeler, Cambridge University Press
dc.identifierhttps://arxiv.org/abs/astro-ph/0403195
dc.identifierhttp://arxiv.org/abs/astro-ph/0403195
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7491
dc.subjectAstrophysics
dc.titleThe Evolution of Supernovae in the Winds of Massive Stars
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