The infancy of supernova remnants: evolving a supernova into its remnant in 3D

Recently, first neutrino-driven supernova explosions have been obtained in 3D, self-consistent, first-principle simulations, these models are still not always exploding robustly and, in general, the explosions are not sufficiently energetic. To constrain the explosion mechanism, and the related unce...

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Veröffentlicht in:	Proceedings of the International Astronomical Union 2017-02, Vol.12 (S331), p.141-147
Hauptverfasser:	Gabler, Michael, Janka, Hans-Thomas, Wongwathanarat, Annop
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Beta decay Computer simulation Contributed Papers Ejecta Ejection Explosions Simulation Stellar evolution Supernova remnants Supernovae Three dimensional models X-rays
Online-Zugang:	Volltext
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