Variable very-high-energy gamma-ray emission from the microquasar LS I +61 303

dc.creatorAlbert, J.
dc.creatorAliu, E.
dc.creatorAnderhub, H.
dc.creatorAntoranz, P.
dc.creatorArmada, A.
dc.creatorAsensio, M.
dc.creatorBaixeras, C.
dc.creatorBarrio, J. A.
dc.creatorBartelt, M.
dc.creatorBartko, H.
dc.creatorBastieri, D.
dc.creatorBavikadi, S. R.
dc.creatorBednarek, W.
dc.creatorBerger, K.
dc.creatorBigongiari, C.
dc.creatorBiland, A.
dc.creatorBisesi, E.
dc.creatorBock, R. K.
dc.creatorBordas, P.
dc.creatorBosch Ramon, Valentí
dc.creatorBretz, T.
dc.creatorBritvitch, I.
dc.creatorCamara, M.
dc.creatorCarmona, E.
dc.creatorChilingarian, A.
dc.creatorCiprini, S.
dc.creatorCoarasa, J. A.
dc.creatorRomero, Gustavo Esteban
dc.creatorRügamer, S.
dc.creatorTorres, Diego F.
dc.date.accessioned2017-11-30T14:53:03Z
dc.date.accessioned2018-11-06T15:43:53Z
dc.date.available2017-11-30T14:53:03Z
dc.date.available2018-11-06T15:43:53Z
dc.date.created2017-11-30T14:53:03Z
dc.date.issued2006-06
dc.identifierAlbert, J.; Aliu, E.; Anderhub, H.; Antoranz, P.; Armada, A.; et al.; Variable very-high-energy gamma-ray emission from the microquasar LS I +61 303; American Association for the Advancement of Science; Science; 312; 5781; 6-2006; 1771-1773
dc.identifier0036-8075
dc.identifierhttp://hdl.handle.net/11336/29324
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1900321
dc.description.abstractMicroquasars 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 gamma-ray emission above 100 gigaelectron volts from the microquasar LS I +61 303. Six orbital cycles were recorded. Several detections occur at a similar orbital phase, which suggests that the emission is periodic. The strongest gamma-ray emission is not observed when the two stars are closest to one another, implying a strong orbital modulation of the emission or absorption processes.
dc.languageeng
dc.publisherAmerican Association for the Advancement of Science
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://www.sciencemag.org/content/312/5781/1771.full
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/ 10.1126/science.1128177
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectMicroquasars
dc.subjectBinary stars
dc.subjectCosmic rays
dc.subjectLS I +61 303 (microcuásar)
dc.titleVariable very-high-energy gamma-ray emission from the microquasar LS I +61 303
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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