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Utilizing Supernova Remnants as Probes of Explosion Mechanisms and Progenitor Systems

Published online by Cambridge University Press:  27 October 2016

Dan Milisavljevic
Dan Milisavljevic*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA, 02138 email: dmilisav@cfa.harvard.edu
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Abstract

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Theory and observation strongly favor the notion that asymmetric explosions drive core-collapse supernovae, but where and how this asymmetry becomes introduced is uncertain. The most likely places of origin are in the explosion mechanism itself or the interior structure of the star into which the explosion proceeds. Investigating the recently uncovered bubble-like interiors of young, nearby supernova remnants may provide a way to unravel which of these competing processes dominate.

Keywords

supernovae: generalsupernova remnnats
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 225 - 226
Copyright
Copyright © International Astronomical Union 2016 

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