Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities

ABSTRACT The reverse shock in the ejecta of core-collapse supernovae is potentially able to destroy newly formed dust material. In order to determine dust survival rates, we have performed a set of hydrodynamic simulations using the grid-based code astrobear in order to model a shock wave interactin...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society Jg. 489; H. 4; S. 4465 - 4496
Hauptverfasser:	Kirchschlager, Florian, Schmidt, Franziska D, Barlow, M J, Fogerty, Erica L, Bevan, Antonia, Priestley, Felix D
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	United Kingdom Oxford University Press 11.11.2019 Royal Astronomical Society
Schlagworte:	ASTRONOMY AND ASTROPHYSICS dust, extinction hydrodynamics ISM: supernova remnants methods: numerical shock waves supernovae: general supernovae: individual: Cassiopeia A ISM: supernova remnants dust, extinction supernovae: individual: Cassiopeia A hydrodynamics methods: numerical supernovae: general shock waves
ISSN:	0035-8711, 1365-2966
Online-Zugang:	Volltext
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