Recollimation and Radiative Focusing of Relativistic Jets: Applications to Blazars and M87
arXiv:0810.0562 · doi:10.1088/0004-637X/699/2/1274
Abstract
Recent observations of M87 and some blazars reveal violent activity in small regions located at relatively large distances from the central engine. Motivated by these considerations, we study the hydrodynamic collimation of a relativistic cooling outflow using a semi-analytical model developed earlier. We first demonstrate that radiative cooling of the shocked outflow layer can lead to a focusing of the outflow and its reconfinement in a region having a very small cross-sectional radius. Such a configuration can produce rapid variability at large distances from the central engine via reflections of the converging recollimation shock. Possible applications of this model to TeV blazars are discussed. We then apply our model to M87. The low radiative efficiency of the M87 jet renders focusing unlikely. However, the shallow profile of the ambient medium pressure inferred from observations, results in extremely good collimation that can explain the reported variability of the X-ray flux emitted from the HST-1 knot.
17 pages, 4 figures. Accepted by ApJ
References in corpus (7)
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- Gamma-ray Flare of PKS 1222+216 in 2010: Effect of Jet Dynamics at the Recollimation Zone
- Probing the central black hole in M87 with gamma-rays
- Multi-Wavelength Polarimetry and Spectral Study of M87 Jet During 2002-2008
- Reconfinement of highly magnetized jets: Implications for HST-1 in M87
- Modeling the spectral-energy-distribution of 3C 454.3 in a "flat" broad-line-region scenario