On the evolution of supernova remnants. III - Off-centred supernova explosions in pre-existing wind-driven bubbles

Bibcode
1993MNRAS.261..674R
Rozyczka, M.; Tenorio-Tagle, G.; Franco, J.; Bodenheimer, P.
Bibliographical reference

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 3, p. 674-680.

Advertised on:
4
1993
Number of authors
4
IAC number of authors
2
Citations
40
Refereed citations
34
Description
It is shown that supernova explosions inside wind-driven cavities created by progenitors moving across the ambient medium result in a large diversity of remnant structures. In particular, barrel-like remnants can be explained as a result of an off-centered explosion within an almost spherical cavity, whereas explosions in strongly elongated cavities produce remnants showing transient jet-like features.
Type
Refereed
Stellar evolution
Stellar winds
Supernova remnants

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