The beaming pattern of external compton emission from relativistic outflows: The case of anisotropic distribution of electrons

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Abstract

The beaming pattern of radiation emitted by a relativistically moving source, such as jets in microquasars, active galactic nuclei, and gamma-ray bursts, is a key issue for understanding acceleration and radiation processes in these objects. In this paper, we introduce a formalism based on a solution of the photon transfer equation to study the beaming patterns for emission produced by electrons accelerated in the jet and the upscattering photons of low-energy radiation fields of external origin (the so-called external Compton scenario). The formalism allows us to treat non-stationary, non-homogeneous, and anisotropic distributions of electrons, but assuming homogeneous/isotropic and non-variable target photon fields. We demonstrate the non-negligible impact of the anisotropy in the electron distribution on angular and spectral characteristics of the EC radiation. © 2014. The American Astronomical Society. All rights reserved..

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Kelner, S. R., Lefa, E., Rieger, F. M., & Aharonian, F. A. (2014). The beaming pattern of external compton emission from relativistic outflows: The case of anisotropic distribution of electrons. Astrophysical Journal, 785(2). https://doi.org/10.1088/0004-637X/785/2/141

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