Relativistic electron beams in IDV blazars
| dc.creator | Crusius-W"atzel, A. R. | |
| dc.creator | Lesch, H. | |
| dc.date | 1998-07-20 | |
| dc.date.accessioned | 2026-07-07T02:27:26Z | |
| dc.date.available | 2026-07-07T02:27:26Z | |
| dc.description | The observed variability of BL Lac objects and Quasars on timescales <1 day (intraday variability, IDV) have revealed radio brightness temperatures up to 10^{16}-10^{20} K. These values challenge the beaming model with isotropic comoving radio emission beyond its limits, requiring bulk relativistic motion with Lorentz factors >100. We argue in favor of a model where an anisotropic distribution of relativistic electrons streams out along the field lines. When this relativistic beam is scattered in pitch angle and/or hits a magnetic field with components perpendicular to the beam velocity it starts to emit synchrotron radiation and redistribute in momentum space. The propagation of relativistic electrons with Lorentz factor gamma=10^2-10^4 reduces the intrinsic variability timescale by a factor gamma^{-1}, so that the intrinsic brightness temperature is reduced by a factor of order gamma^{-2}, easily below the Inverse Compton limit of 10^{12} K. When looking at a single event we expect the variability time scales to be independent of frequency for a monoenergetic electron beam. The production of variable X- and gamma-ray flux is briefly discussed. | |
| dc.description | 6 pages, to be published in "Astronomy and Astrophysics" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9807196 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9807196 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12689 | |
| dc.subject | Astrophysics | |
| dc.title | Relativistic electron beams in IDV blazars | |
| dc.type | text |