The infancy of core-collapse supernova remnants

ABSTRACT We present 3D hydrodynamic simulations of neutrino-driven supernovae (SNe) with the Prometheus-HotB code, evolving the asymmetrically expanding ejecta from shock breakout until they reach the homologous expansion phase after roughly one year. Our calculations continue the simulations for tw...

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Bibliographic Details

Published in:	Monthly notices of the Royal Astronomical Society Vol. 502; no. 3; pp. 3264 - 3293
Main Authors:	Gabler, Michael, Wongwathanarat, Annop, Janka, Hans-Thomas
Format:	Journal Article
Language:	English
Published:	Oxford University Press 01.04.2021
Subjects:	stars: massive supernovae: general ISM: supernova remnants
ISSN:	0035-8711, 1365-2966
Online Access:	Get full text
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