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- W2023508189 abstract "Abstract Systems of two very different sizescales are known to produce very high-energy (VHE) radiation in their jets: AGNs and microquasars. The produced VHE photons ( E γ ~ 1 TeV) can be absorbed by the intense environmental soft photon fields, coming from the companion star (in high mass binaries) or from the accreting material (disk+corona in AGNs), as these are the dominant sources at energies around ~( m e c 2 ) 2 / E γ . Energetic pairs are created by the photon-photon annihilation, and, depending on how efficient are the competing cooling channels, the absorption can lead to a reprocessing by Inverse Compton pair-cascade development. A self-consistent modeling of these systems as gamma-ray sources should then include, along with the emission and absorption processes, a thorough treatment of the pair cascades. We discuss here on this issue, focusing on our (preliminary) results of numerical simulations devoted to a study case similar to the high-mass microquasar candidate LS 5039." @default.
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- W2023508189 date "2010-09-01" @default.
- W2023508189 modified "2023-09-27" @default.
- W2023508189 title "On the reprocessing of gamma-rays produced by jets" @default.
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- W2023508189 doi "https://doi.org/10.1017/s1743921310015723" @default.
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