Interaction of supernova blast waves with wind-driven shells: formation of "jets", "bullets", "ears", etc

dc.creatorGvaramadze, V. V.
dc.date1999-12-24
dc.date.accessioned2026-07-07T02:35:12Z
dc.date.available2026-07-07T02:35:12Z
dc.descriptionMost of middle-aged supernova remnants (SNRs) have a distorted and complicated appearance which cannot be explained in the framework of the Sedov-Taylor model. We consider three typical examples of such SNRs (Vela SNR, MSH 15-52, G 309.2-00.6) and show that their structure could be explained as a result of interaction of a supernova (SN) blast wave with the ambient medium preprocessed by the action of the SN progenitor's wind and ionized emission.
dc.description4 pages, talk given at the Gamov Memorial International Conference "The Universe of Gamow: Original Ideas in Astrophysics and Cosmology", Odessa, August 16-22, 1999; to appear in Odessa Astronomical Publications, 1999, vol. 12
dc.identifierhttps://arxiv.org/abs/astro-ph/9912512
dc.identifierhttp://arxiv.org/abs/astro-ph/9912512
dc.identifierOdessa Astron. Publ., 12 (1999) 117
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15524
dc.subjectAstrophysics
dc.titleInteraction of supernova blast waves with wind-driven shells: formation of "jets", "bullets", "ears", etc
dc.typetext

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