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dc.creatorSupanitsky, Alberto Daniel-
dc.creatorde Souza, V.-
dc.date2017-05-29T18:31:15Z-
dc.date2017-05-29T18:31:15Z-
dc.date2013-12-
dc.date2017-05-23T19:16:28Z-
dc.date.accessioned2019-04-29T15:52:52Z-
dc.date.available2019-04-29T15:52:52Z-
dc.date.issued2013-12-
dc.identifierSupanitsky, Alberto Daniel; de Souza, V.; An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations; Iop Publishing; Journal Of Cosmology And Astroparticle Physics; 2013; 12-2013; 231-17-
dc.identifier1475-7516-
dc.identifierhttp://hdl.handle.net/11336/17074-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/304485-
dc.descriptionDifferent types of extragalactic objects are known to produce TeV gamma-rays. Some of these objects are the most probable candidates to accelerate cosmic rays up to 1020 eV. It is very well known that gamma-rays can be produced as a result of the cosmic ray propagation through the intergalactic medium. These gamma-rays contribute to the total flux observed in the direction of the source. In this paper we propose a new method to derive an upper limit on the cosmic-ray luminosity of an individual source based on the measured upper limit on the integral flux of GeV-TeV gamma-rays. We show how it is possible to calculate an upper limit on the cosmic-ray luminosity of a particular source and we explore the parameter space in which the current GeV-TeV gamma-ray measurements can offer a useful determination. We study in detail two particular sources, Pictor A and NGC 7469, and we calculate the upper limit on the proton luminosity of each source based on the upper limit on the integral gamma-ray flux measured by the H.E.S.S. telescopes.-
dc.descriptionFil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina-
dc.descriptionFil: de Souza, V.. Universidade de Sao Paulo; Brasil-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherIop Publishing-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/1475-7516/2013/12/023-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/iopscience.iop.org/article/10.1088/1475-7516/2013/12/023-
dc.relationinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1311.4820-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.subjectultra high energy cosmic rays-
dc.subjectgamma ray experiments-
dc.subjectgamma ray theory-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleAn upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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