Buscar
Mostrando ítems 1-7 de 7
Hadronic high-energy gamma ray emission from microquasars
(IOP Publishing, 2005-06)
We present a hadronic model for gamma-ray production in the microquasar LS I +61 303. The system is formed by a neutron star that accretes matter from the dense and slow equatorial wind of the Be primary star. We calculate ...
Towards a population of HMXB/NS microquasars as counterparts of low-latitude unidentified EGRET sources
(Springer, 2005-12)
The discovery of the microquasar LS 5039 well within the 95% confidence contour of the Unidentified EGRET Source (UES) 3EG J1824‑1514 was a major step towards the possible association between microquasars (MQs) and UESs. ...
Variable very-high-energy gamma-ray emission from the microquasar LS I +61 303
(American Association for the Advancement of Science, 2006-06)
Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sources of cosmic rays and can be used to elucidate the physics of relativistic jets. We report the detection of variable ...
Hadronic gamma-ray production in microquasars with equatorial winds
(Universidad Nacional Autónoma de México. Instituto de Astronomía, 2006-12)
Los microcuasáres son sistemas binarios con emisión en rayos X vinculada a acreción, en los cuales se han detectado chorros de partículas relativistas (jets) a través de su emisión en bandas de radio. La transferencia de ...
Jet interactions in massive X-ray binaries
(Universidad Nacional Autónoma de México. Instituto de Astronomía, 2008-12)
Los sistemas binarios masivos de rayos X están formados por un objeto compacto que acreta materia del viento estelar de una estrella donante de tipo temprano. En algunos de estos sistemas, llamados microcuásares, chorros ...