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, 1993 Considering shock-accelerated protons in addition to electrons in a synchrotron radio jet naturally produces the observed X- through gamma ray continuum emission of flat-spectrum radio-loud AGN, whereas the corresponding shock-accelerated electrons produce the infrared through optical continuum.
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Temporal and Spectral Variabilities of High‐Energy Emission from Blazars Using Synchrotron Self‐Compton Models [PDF]
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