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Hydrodynamical instability of extragalactic stratified jets

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dc.contributor.author Hanasz, Michał
dc.contributor.author Sol, Helene
dc.date.accessioned 2012-12-19T09:06:13Z
dc.date.available 2012-12-19T09:06:13Z
dc.date.issued 1997-11-20
dc.identifier.uri http://repozytorium.umk.pl/handle/item/256
dc.description.abstract The recent development of tomographic analysis of radio data shows the presence of sheaths around several extragalactic jets. We have studied the Kelvin-Helmholtz instability of such stratified jets, describing them as inner relativistic beams embedded in slower plasma envelopes. We find that the para- meters of the envelope generally determine the Kelvin-Helmholtz properties of the jet which thus appears isolated from any ambient external medium.
dc.language.iso eng
dc.relation.uri http://arxiv.org/abs/astro-ph/9711240
dc.rights info:eu-repo/semantics/openAccess
dc.subject Astrophysics
dc.title Hydrodynamical instability of extragalactic stratified jets
dc.type info:eu-repo/semantics/article


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