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• W2056577833 abstract "We present the basic equations for calculating the time-dependent received spectral flux from the optically thin emissivities produced by temporally evolving, nonthermal electrons losing energy in a relativistically moving blob of plasma located at cosmological distances. Ionization, bremsstrahlung, Compton, and synchrotron energy losses of the electrons are considered. These equations are used to derive and calculate the received spectral fluence produced by instantaneously injected nonthermal electrons that also scatter photons from an isotropic external monochromatic radiation field in the Thomson regime of scattering. The derivation of the fluences is restricted to the regime where either synchrotron losses or Thomson losses with photons of the external radiation field dominate the electron energy loss rate. We also derive approximate expressions for the synchrotron and synchrotron self-Compton fluence. Beaming factors for thin-target and thick-target models of the electron distributions are derived. We show that ionization energy losses of relativistic electrons on the background thermal plasma of the blob can give Comptonized gamma-ray fluence spectra with spectral breaks Δα ≫ 0.5. If only Thomson and synchrotron losses are important, spectral breaks ≫0.5 are also possible if electrons are injected with a low-energy cutoff or if a snapshot of the spectral flux is measured over a time interval much less than the interval during which electrons cool." @default.
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• W2056577833 date "1997-03-01" @default.
• W2056577833 modified "2023-10-16" @default.
• W2056577833 title "Nonthermal Compton and Synchrotron Processes in the Jets of Active Galactic Nuclei" @default.
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• W2056577833 doi "https://doi.org/10.1086/312972" @default.
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