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First Bounds on the High-Energy Emission from Isolated Wolf-Rayet Binary Systems

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dc.contributor.authorMAGIC Collaboration
dc.contributor.authorParedes i Poy, Josep Maria
dc.contributor.authorRibó Gomis, Marc
dc.contributor.authorBosch i Ramon, Valentí
dc.date.accessioned2020-02-13T11:40:10Z
dc.date.available2020-02-13T11:40:10Z
dc.date.issued2008-09-09
dc.date.updated2020-02-13T11:40:10Z
dc.description.abstractHigh-energy gamma-ray emission is theoretically expected to arise in tight binary star systems (with high mass loss and high-velocity winds), although the evidence of this relationship has proven to be elusive so far. Here we present the first bounds on this putative emission from isolated Wolf-Rayet (WR) star binaries, WR 147 and WR 146, obtained from observations with the MAGIC telescope.
dc.format.extent4 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec570854
dc.identifier.issn2041-8205
dc.identifier.urihttps://hdl.handle.net/2445/150123
dc.language.isoeng
dc.publisherInstitute of Physics (IOP)
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1086/592433
dc.relation.ispartofAstrophysical Journal Letters, 2008, vol. 685, num. 1, p. 71-74
dc.relation.urihttps://doi.org/10.1086/592433
dc.rights(c) American Astronomical Society, 2008
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationRaigs gamma
dc.subject.classificationObservacions astronòmiques
dc.subject.otherGamma rays
dc.subject.otherAstronomical observations
dc.titleFirst Bounds on the High-Energy Emission from Isolated Wolf-Rayet Binary Systems
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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