Jet confinement by magneto-torsional oscillations
| dc.creator | Bisnovatyi-Kogan, Gennady | |
| dc.date | 2007-07-01 | |
| dc.date.accessioned | 2026-07-07T10:56:33Z | |
| dc.date.available | 2026-07-07T10:56:33Z | |
| dc.description | Many quasars and active galactic nuclei (AGN) appear in radio, optical, and X-ray maps, as a bright nuclear sources from which emerge single or double long, thin jets. When observed with high angular resolution these jets show structure with bright knots separated by relatively dark regions. Nonthermal nature of a jet radiation is well explained as the synchrotron radiation of the relativistic electrons in an ordered magnetic field. We consider magnetic collimation, connected with torsional oscillations of a cylinder with elongated magnetic field, and periodically distributed initial rotation around the cylinder axis. The stabilizing azimuthal magnetic field is created here by torsional oscillations, where charge separation is not necessary. Approximate simplified model is developed. Ordinary differential equation is derived, and solved numerically, what gives a possibility to estimate quantitatively the range of parameters where jets may be stabilized by torsional oscillations. | |
| dc.description | accepted for publication in Astrophysics and Space Science | |
| dc.identifier | https://arxiv.org/abs/0707.0122 | |
| dc.identifier | http://arxiv.org/abs/0707.0122 | |
| dc.identifier | Astrophys.SpaceSci.311:287-292,2007 | |
| dc.identifier | doi:10.1007/s10509-007-9564-y | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/186447 | |
| dc.subject | Astrophysics | |
| dc.title | Jet confinement by magneto-torsional oscillations | |
| dc.type | text |