Dust destruction by the reverse shock in the clumpy supernova remnant Cassiopeia A based on hydrodynamic simulations

Observations of the ejecta of core-collapse supernovae have shown that dust grains form in over-dense gas clumps in the expanding ejecta. The clumps are later subject to the passage of the reverse shock and a significant amount of the newly formed dust material can be destroyed due to the high tempe...

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Veröffentlicht in:	arXiv.org 2019-09
Hauptverfasser:	Kirchschlager, Florian, Schmidt, Franziska D, Barlow, M J, Fogerty, Erica L, Bevan, Antonia, Priestley, Felix D
Format:	Artikel
Sprache:	eng
Schlagworte:	Cassiopeia A Clumps Collapse Computer simulation Destruction Dust Ejecta Grain size Post-processing Shock waves Space telescopes Supernova remnants Supernovae Survival
Online-Zugang:	Volltext
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