Estimating jet power in proton blazar models

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dc.creatorProtheroe, R. J.
dc.creatorMücke, A.
dc.date2000-10-31
dc.date.accessioned2026-07-07T01:56:18Z
dc.date.available2026-07-07T01:56:18Z
dc.descriptionWe 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.
dc.description4 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0010625
dc.identifierhttp://arxiv.org/abs/astro-ph/0010625
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1949
dc.subjectAstrophysics
dc.titleEstimating jet power in proton blazar models
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