SIMBAD references

2008MNRAS.385..283C - Mon. Not. R. Astron. Soc., 385, 283-300 (2008/March-3)

The power of blazar jets.

CELOTTI A. and GHISELLINI G.

Abstract (from CDS):

We estimate the power of relativistic, extragalactic jets by modelling the spectral energy distribution of a large number of blazars. We adopt a simple one-zone, homogeneous, leptonic synchrotron and inverse Compton model, taking into account seed photons originating both locally in the jet and externally. The blazars under study have an often dominant high-energy component which, if interpreted as due to inverse Compton radiation, limits the value of the magnetic field within the emission region. As a consequence, the corresponding Poynting flux cannot be energetically dominant. Also the bulk kinetic power in relativistic leptons is often smaller than the dissipated luminosity. This suggests that the typical jet should comprise an energetically dominant proton component. If there is one proton per relativistic electrons, jets radiate around 2-10 per cent of their power in high-power blazars and 3-30 per cent in less powerful BL Lacs.

Abstract Copyright: 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): radiation mechanisms: non-thermal - galaxies: active - galaxies: jets

CDS comments: In table A1 : 0234-285 is a misprint for 0234+285, 0827+234 is a misprint for 0827+243.

Simbad objects: 74

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2008MNRAS.385..283C and select 'bookmark this link' or equivalent in the popup menu


2019.10.16-22:59:58

© Université de Strasbourg/CNRS

    • Contact