Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/150123
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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.identifier.issn2041-8205-
dc.identifier.urihttp://hdl.handle.net/2445/150123-
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.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.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-
dc.identifier.idgrec570854-
dc.date.updated2020-02-13T11:40:10Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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