Microquasars and Gamma-ray Sources

dc.creatorRomero, Gustavo Esteban
dc.date.accessioned2017-12-05T14:39:53Z
dc.date.accessioned2018-11-06T12:56:53Z
dc.date.available2017-12-05T14:39:53Z
dc.date.available2018-11-06T12:56:53Z
dc.date.created2017-12-05T14:39:53Z
dc.date.issued2005-12
dc.identifierRomero, Gustavo Esteban; Microquasars and Gamma-ray Sources; Science Press; Chinese Journal of Astronomy and Astrophysics; 5; 12-2005; 110-120
dc.identifier1009-9271
dc.identifierhttp://hdl.handle.net/11336/29696
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1871504
dc.description.abstractMicroquasars are X-ray binary systems with non-thermal radio emission originated in jet-like features. They are attractive sites for gamma-ray production, since relativistic particles in the jet should traverse locally strong both photon and matter fields. In this review we discuss whether some of the unidentified gamma-ray sources detected by the EGRET instrument of the Compton Gamma-Ray Observatory might be associated with microquasars. Relevant models for gamma-ray emission in such binaries are described and prospects for the detection of microquasars with instruments of new generation are briefly evaluated.
dc.languageeng
dc.publisherScience Press
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2005ChJAS...5..110R
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://articles.adsabs.harvard.edu/full/2005ChJAS...5..110R
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectMicroquasars
dc.subjectGamma ray observations
dc.subjectGamma rays
dc.subjectX ray binaries
dc.titleMicroquasars and Gamma-ray Sources
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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