Hydrodynamical instability of extragalactic stratified jets
| dc.creator | Hanasz, M. | |
| dc.creator | Sol, H. | |
| dc.date | 1997-11-20 | |
| dc.date.accessioned | 2026-07-25T20:37:08Z | |
| dc.description | 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.description | LaTeX, 5 pages, 1 figure and crckapb.sty, epsf.sty included, To appear in the proceedings of Girona Conference ``Blazars, Black Holes and Jets'', 9-12 September 1996, Girona, Spain | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9711240 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9711240 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/71937 | |
| dc.subject | Astrophysics | |
| dc.title | Hydrodynamical instability of extragalactic stratified jets | |
| dc.type | text |