On the reprocessing of gamma-rays produced by jets
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 (Eγ ∼ 1 TeV) can be absorbed by the intense environmental soft photon fields, coming from the companion star (in high mass binaries) or from t...
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todo:paper_17439213_v6_nS275_p98_Orellana2023-10-03T16:31:37Z On the reprocessing of gamma-rays produced by jets Orellana, M. Pellizza, L.J. Romero, G.E. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M. Gamma rays: theory Radiation mechanisms: nonthermal 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 (Eγ ∼ 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 ∼ (me c2 ) 2/Eγ . Energetic pairs are created by the photonphoton 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 selfconsistent 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. © International Astronomical Union 2011. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS275_p98_Orellana |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Gamma rays: theory Radiation mechanisms: nonthermal |
spellingShingle |
Gamma rays: theory Radiation mechanisms: nonthermal Orellana, M. Pellizza, L.J. Romero, G.E. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M. On the reprocessing of gamma-rays produced by jets |
topic_facet |
Gamma rays: theory Radiation mechanisms: nonthermal |
description |
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 (Eγ ∼ 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 ∼ (me c2 ) 2/Eγ . Energetic pairs are created by the photonphoton 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 selfconsistent 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. © International Astronomical Union 2011. |
format |
SER |
author |
Orellana, M. Pellizza, L.J. Romero, G.E. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M. |
author_facet |
Orellana, M. Pellizza, L.J. Romero, G.E. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M. |
author_sort |
Orellana, M. |
title |
On the reprocessing of gamma-rays produced by jets |
title_short |
On the reprocessing of gamma-rays produced by jets |
title_full |
On the reprocessing of gamma-rays produced by jets |
title_fullStr |
On the reprocessing of gamma-rays produced by jets |
title_full_unstemmed |
On the reprocessing of gamma-rays produced by jets |
title_sort |
on the reprocessing of gamma-rays produced by jets |
url |
http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS275_p98_Orellana |
work_keys_str_mv |
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1807319048867807232 |