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pγ interactions in Galactic jets as a plausible origin of the positron excess

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dc.contributor.authorGupta, Nayantara
dc.contributor.authorTorres, Diego F.
dc.date.accessioned2014-09-11T12:25:37Z
dc.date.available2014-09-11T12:25:37Z
dc.date.issued2014-07-04
dc.descriptionOpen Access.en
dc.description.abstractThe positron flux measured near Earth shows a rise with energy beyond 30 GeV. We show that this rise might be compatible with the production of positrons in pγ interactions in the jets of microquasars.en
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2014, Vol. 441, p3122-3126en
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966 - (online)
dc.identifier.urihttp://hdl.handle.net/2289/5968
dc.language.isoenen
dc.publisherOxford University Pressen
dc.relation.urihttp://adsabs.harvard.edu/abs/2014MNRAS.441.3122Gen
dc.relation.urihttp://arxiv.org/abs/1404.4188en
dc.relation.urihttp://dx.doi.org/10.1093/mnras/stu770en
dc.rights2014 The authors & the Royal Astronomical Societyen
dc.subjectCosmic raysen
dc.subjectGalaxy centreen
dc.titlepγ interactions in Galactic jets as a plausible origin of the positron excessen
dc.typeArticleen

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