Please use this identifier to cite or link to this item:
http://hdl.handle.net/2445/45384
Title: | AGNs and microquasars as high-energy gamma-ray sources |
Author: | Paredes i Poy, Josep Maria |
Keywords: | Estels binaris de raigs X Raigs gamma Astronomia de raigs gamma Quàsars X-ray binaries Gamma rays Gamma ray astronomy Quasars |
Issue Date: | 2005 |
Publisher: | Springer Science + Business Media |
Abstract: | The possible associations between the microquasars LS 5039 and LS I +61 303 and the EGRET sources 3EG J1824-1514 and 3EG J0241+6103 suggest that microquasars could also be sources of high-energy gamma-rays. In this work, we present a detailed numerical inverse Compton (IC) model, based on a microquasar scenario, that reproduces the high-energy gamma-ray spectra and variability observed by EGRET for the mentioned sources. Our model considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet that interact through IC scattering with both the radiation and the magnetic fields. |
Note: | Versió postprint del document publicat a: http;//dx.doi.org/10.1007/s10509-005-1177-8 |
It is part of: | Astrophysics and Space Science, 2005, vol. 300, num. 1-3, p. 267-274 |
URI: | http://hdl.handle.net/2445/45384 |
Related resource: | http://dx.doi.org/10.1007/s10509-005-1177-8 |
ISSN: | 0004-640X |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
File | Description | Size | Format | |
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546712.pdf | 115.42 kB | Adobe PDF | View/Open |
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