Estimating jet power in proton blazar models
Astrophysics
2007-05-23 v1
Abstract
We discuss the various contributions to the jet luminosity in proton blazar models of active galactic nuclei and describe a method of estimating the jet luminosity from the observed spectral energy distribution (SED) and the fitted model parameters. We apply this to a synchrotron proton blazar (SPB) model for Markarian 501.
Cite
@article{arxiv.astro-ph/0010625,
title = {Estimating jet power in proton blazar models},
author = {R. J. Protheroe and A. Mücke},
journal= {arXiv preprint arXiv:astro-ph/0010625},
year = {2007}
}
Comments
4 pages, 1 figure, to appear in `Particles and Fields in Radio Galaxies', Oxford Radio Galaxy Workshop 2000, ASP Conf. Ser., eds. Robert A. Laing and Katherine M. Blundell