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Linking three-dimensional core-collapse supernova simulations with observations
Published online by Cambridge University Press: 17 October 2017
Abstract
To understand a wide variety of properties of young core-collapse supernova (CCSN) remnants being revealed by modern observations three-dimensional simulations of CCSNe starting from the initiation of the explosion until the expanding stellar debris transform into gaseous remnants are needed. We briefly review recent progress in modeling CCSNe on a long time scale. A current effort to model bolometric light curves based on 3D CCSN explosion models for comparison with observational data from SN 1987A is also discussed.
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- Copyright © International Astronomical Union 2017