Please use this identifier to cite or link to this item:
http://hdl.handle.net/2445/45339
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Bosch i Ramon, Valentí | - |
dc.contributor.author | Paredes i Poy, Josep Maria | - |
dc.date.accessioned | 2013-08-01T11:15:32Z | - |
dc.date.available | 2013-08-01T11:15:32Z | - |
dc.date.issued | 2004 | - |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.uri | http://hdl.handle.net/2445/45339 | - |
dc.description.abstract | The possible association between the microquasar LS 5039 and the EGRET source 3EG J1824-1514 suggests that microquasars could also be sources of high energy gamma-rays. In this paper, we explore, with a detailed numerical model, if this system can produce the emission detected by EGRET (>100 MeV) through inverse Compton (IC) scattering. Our numerical approach considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet, interacting with both the radiation and the magnetic fields, taking into account the Thomson and Klein-Nishina regimes of interaction. The computed spectrum reproduces the observed spectral characteristics at very high energy. | - |
dc.format.extent | 14 p. | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | - |
dc.publisher | Springer Verlag | - |
dc.relation.isformatof | Versió postprint del document publicat a: http://dx.doi.org/10.1051/0004-6361:20035615 | - |
dc.relation.ispartof | Astronomy and Astrophysics, 2004, vol. 417, num. 3, p. 1075-1081 | - |
dc.relation.uri | http://dx.doi.org/10.1051/0004-6361:20035615 | - |
dc.rights | (c) Springer Verlag, 2004 | - |
dc.source | Articles publicats en revistes (Física Quàntica i Astrofísica) | - |
dc.subject.classification | Estels binaris de raigs X | - |
dc.subject.classification | Raigs gamma | - |
dc.subject.classification | Radioastronomia | - |
dc.subject.classification | Astrofísica | - |
dc.subject.other | X-ray binaries | - |
dc.subject.other | Gamma rays | - |
dc.subject.other | Radio astronomy | - |
dc.subject.other | Astrophysics | - |
dc.title | A numerical model for the gamma-ray emission of the microquasar LS 5039 | - |
dc.type | info:eu-repo/semantics/article | - |
dc.type | info:eu-repo/semantics/acceptedVersion | - |
dc.identifier.idgrec | 515495 | - |
dc.date.updated | 2013-08-01T11:15:32Z | - |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | - |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
515495.pdf | 204.22 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.