Please use this identifier to cite or link to this item:
https://hdl.handle.net/2445/45391
Title: | High-energy gamma-ray emission from microquasars: LS 5039 and LS I+61303 |
Author: | Bosch i Ramon, Valentí Paredes i Poy, Josep Maria |
Keywords: | Estels binaris de raigs X Estels Raigs gamma Astronomia de raigs X Astrofísica X-ray binaries Stars Gamma rays X-ray astronomy Astrophysics |
Issue Date: | 2005 |
Publisher: | Chinese Academy of Sciences |
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/10.1088/1009-9271/5/S1/133 |
It is part of: | Chinese Journal of Astronomy and Astrophysics, 2005, vol. 5, p. 133-138 |
URI: | https://hdl.handle.net/2445/45391 |
Related resource: | http://dx.doi.org/10.1088/1009-9271/5/S1/133 |
ISSN: | 1009-9271 |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
File | Description | Size | Format | |
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517654.pdf | 133.32 kB | Adobe PDF | View/Open |
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