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dc.date.accessioned | 2021-09-15T14:55:59Z | |
dc.date.available | 2021-09-15T14:55:59Z | |
dc.date.issued | 2005 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/124871 | |
dc.description.abstract | Microquasars are sources of very high-energy gamma-rays and, very probably, highenergy gamma-ray emitters. We propose a model for a jet that can allow to give accurate observational predictions for jet emission at different energies and provide with physical information of the object using multiwavelength data. | en |
dc.format.extent | 91-92 | es |
dc.language | en | es |
dc.subject | X-rays: binaries | es |
dc.subject | Gamma rays: theory | es |
dc.subject | Gamma rays: observations | es |
dc.title | Leptonic emission from microquasar jets: from radio to very high-energy gamma-rays | en |
dc.type | Articulo | es |
sedici.identifier.other | arXiv:astro-ph/0605466 | es |
sedici.identifier.other | doi:10.1017/s1743921306007976 | es |
sedici.identifier.issn | 1743-9213 | es |
sedici.identifier.issn | 1743-9221 | es |
sedici.creator.person | Bosch Ramon, V. | es |
sedici.creator.person | Paredes, J. M. | es |
sedici.creator.person | Romero, Gustavo Esteban | es |
sedici.subject.materias | Ciencias Astronómicas | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Instituto Argentino de Radioastronomía | es |
sedici.subtype | Comunicacion | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.relation.event | IAU Symposium 230 (Dublin, Ireland, 15-19 August, 2005) | es |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Proceedings of the International Astronomical Union | es |
sedici.relation.journalVolumeAndIssue | vol. 1, no. S230 | es |