Gamma-rays from the compact colliding wind region in Cyg OB2 #5

dc.contributorAharonian, Felix A.
dc.contributorHofmann, Werner
dc.contributorRieger, Frank M.
dc.creatorAraudo, Anabella Teresa
dc.creatorOrtiz Leon, Gisella
dc.creatorRodríguez, Luis Felipe
dc.date.accessioned2022-02-24T12:08:15Z
dc.date.accessioned2022-10-15T12:40:17Z
dc.date.available2022-02-24T12:08:15Z
dc.date.available2022-10-15T12:40:17Z
dc.date.created2022-02-24T12:08:15Z
dc.date.issued2012
dc.identifierGamma-rays from the compact colliding wind region in Cyg OB2 #5; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 422-425
dc.identifier9780735411234
dc.identifierhttp://hdl.handle.net/11336/152650
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4387132
dc.description.abstractIn this contribution we model the non-thermal emission (from radio toγ-rays) produced in the compact (and recently detected) collidingwind region in the multiple stellar system Cyg OB2 #5. We focus ourstudy on the detectability of the produced γ-rays.
dc.languageeng
dc.publisherAmerican Institute of Physics
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4772287
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1063/1.4772287
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.sourceAIP Conference Proceedings
dc.subjectSTARS: BINARIES
dc.subjectSTARS: INDIVIDUAL; CYG OB2 5
dc.subjectRADIATION MECHANISMS: NON THERMAL
dc.subjectGAMMA RAYS: THEORY
dc.titleGamma-rays from the compact colliding wind region in Cyg OB2 #5
dc.typeinfo:eu-repo/semantics/publishedVersion
dc.typeinfo:eu-repo/semantics/conferenceObject
dc.typeinfo:ar-repo/semantics/documento de conferencia


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