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Evolution of supernovae in the winds of massive stars

Published online by Cambridge University Press:  26 May 2016

Vikram V. Dwarkadas
Vikram V. Dwarkadas*
Affiliation:
Bartol Research Institute, University of Delaware, 217 Sharp Laboratory, Newark, DE 19350, USA

Abstract

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Core-collapse supernovae (SNe) arise from massive stars, which lose mass in the form of stellar winds throughout their lifetimes. We study herein the evolution of the SNe as they grow in the circumstellar medium formed by mass loss from the progenitor star.

Type
Part 4. Feedback from Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 710 - 711
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Dwarkadas, V.V. 2001, J. Korean Astron. Soc. 34, 243.Google Scholar
Dwarkadas, V.V. 2002, in: Moffat, A.F.J. & St-Louis, N. (eds.), Interacting Winds from Massive Stars, ASP-CS 260, 141,Google Scholar
Weaver, R.P., McCray, R., Castor, J.I., Shapiro, P.R., Moore, R.L. 1977, ApJ 218, 377.Google Scholar