Estimating jet power in proton blazar models
classification
🌌 astro-ph
keywords
blazarprotonestimatingluminositymodelmodelsactiveapply
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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.
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