| dc.creator | Orellana, Mariana Dominga | |
| dc.creator | Pellizza, L. J. | |
| dc.creator | Romero, Gustavo Esteban | |
| dc.date | 2010 | |
| dc.date | 2019-10-02T13:50:06Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/82474 | |
| dc.identifier | issn:17439213 | |
| dc.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 ∼ (m<SUB>e</SUB> c<SUP>2</SUP> ) <SUP>2</SUP>/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. | |
| dc.description | Facultad de Ciencias Astronómicas y Geofísicas | |
| dc.format | application/pdf | |
| dc.format | 98-99 | |
| dc.language | en | |
| dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
| dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
| dc.subject | Ciencias Astronómicas | |
| dc.subject | Gamma rays: theory | |
| dc.subject | Radiation mechanisms: nonthermal | |
| dc.title | On the reprocessing of gamma-rays produced by jets | |
| dc.type | Articulo | |
| dc.type | Comunicacion | |
