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Linking three-dimensional core-collapse supernova simulations with observations

Published online by Cambridge University Press:  17 October 2017

Annop Wongwathanarat Open the ORCID record for Annop Wongwathanarat [Opens in a new window]
Annop Wongwathanarat*
Affiliation:
RIKEN, Astrophysical Big Bang Laboratory, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan email: annop.wongwathanarat@riken.jp Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany
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Abstract

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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.

Keywords

supernovae: generalsupernovae: individual (Supernova 1987A)hydrodynamicsinstabilities
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S331: Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their aftermaths , February 2017 , pp. 101 - 106
Copyright
Copyright © International Astronomical Union 2017 

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