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dc.contributor.authorHOPPE, S.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorLEMOINE-GOUMARD, M.
dc.date.issued2008
dc.date.conference2007-07-03
dc.description.abstractEnThe shell-type supernova remnant (SNR) RCW 86 - possibly associated with the historical supernova SN 185 - was observed during the past three years with the High Energy Stereoscopic System (H.E.S.S.), an array of four atmospheric-Cherenkov telescopes located in Namibia. The multi-wavelength properties of RCW 86, e.g. weak radio emission and North-East X-ray emission almost entirely consisting of synchroton radiation, resemble those of two very-high energy (VHE; > 100 GeV) gamma-ray emitting SNRs RX J1713.7-3946 and RX J0852-4622. The H.E.S.S. observations reveal a new extended source of VHE gamma-ray emission.The morphological and spectral properties of this new source will be presented.
dc.language.isoen
dc.source.titleProceedings of the 30th International Cosmic Ray Conference
dc.title.enH.E.S.S. observations of the supernovae remnant RCW 86
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv0709.4103
bordeaux.page585-588
bordeaux.volume2
bordeaux.countryMX
bordeaux.title.proceedingProceedings of the 30th International Cosmic Ray Conference
bordeaux.conference.cityMerida
bordeaux.peerReviewedoui
hal.identifierin2p3-00319902
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2007-07-11
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00319902v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=Proceedings%20of%20the%2030th%20International%20Cosmic%20Ray%20Conference&rft.date=2008&rft.volume=2&rft.spage=585-588&rft.epage=585-588&rft.au=HOPPE,%20S.&LEMOINE-GOUMARD,%20M.&rft.genre=unknown


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