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hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorGUILLEMOT, L.
dc.contributor.authorJ. JOHNSON, T.
dc.contributor.authorVENTER, C.
hal.structure.identifierDepartment of Geophysics [Stanford]
dc.contributor.authorKERR, M.
hal.structure.identifierMoredun Research Institute [Penicuik, UK] [MRI]
dc.contributor.authorLIVINGSTONE, M.
dc.contributor.authorH. JANSSEN, G.
dc.contributor.authorJAROENJITTICHAI, P.
dc.contributor.authorKRAMER, M.
dc.contributor.authorW. STAPPERS, B.
dc.contributor.authorK. HARDING, A.
dc.contributor.authorCAMILO, F.
dc.contributor.authorM. ESPINOZA, C.
dc.contributor.authorC. C. FREIRE, P.
dc.contributor.authorGARGANO, F.
dc.contributor.authorE. GROVE, J.
dc.contributor.authorJOHNSTON, S.
dc.contributor.authorF. MICHELSON, P.
dc.contributor.authorNOUTSOS, A.
dc.contributor.authorPARENT, D.
dc.contributor.authorM. RANSOM, S.
dc.contributor.authorS. RAY, P.
dc.contributor.authorSHANNON, R.
dc.contributor.authorE. THORSETT, S.
dc.contributor.authorWEBB, N.
dc.contributor.authorJOHNSON, T. J.
dc.contributor.authorJANSSEN, G.
dc.contributor.authorKRÄMER, M.
hal.structure.identifierJodrell Bank Centre for Astrophysics
dc.contributor.authorSTAPPERS, B. W.
dc.contributor.authorHARDING, A.
dc.contributor.authorESPINOZA, C. M.
dc.contributor.authorFREIRE, P. C. C.
dc.contributor.authorGROVE, J. E.
dc.contributor.authorMICHELSON, P. F.
dc.contributor.authorRANSOM, S. M.
dc.contributor.authorRAY, P. S.
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
dc.contributor.authorTHEUREAU, Gilles
dc.contributor.authorTHORSETT, S. E.
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
dc.contributor.authorCOGNARD, Ismael
dc.date.issued2012
dc.identifier.issn0004-637X
dc.description.abstractEnWe report the detection of pulsed gamma-ray emission from the fast millisecond pulsars (MSPs) B1937+21 (also known as J1939+2134) and B1957+20 (J1959+2048) using 18 months of survey data recorded by the \emph{Fermi} Large Area Telescope (LAT) and timing solutions based on radio observations conducted at the Westerbork and Nançay radio telescopes. In addition, we analyzed archival \emph{RXTE} and \emph{XMM-Newton} X-ray data for the two MSPs, confirming the X-ray emission properties of PSR B1937+21 and finding evidence ($\sim 4\sigma$) for pulsed emission from PSR B1957+20 for the first time. In both cases the gamma-ray emission profile is characterized by two peaks separated by half a rotation and are in close alignment with components observed in radio and X-rays. These two pulsars join PSRs J0034-0534 and J2214+3000 to form an emerging class of gamma-ray MSPs with phase-aligned peaks in different energy bands. The modeling of the radio and gamma-ray emission profiles suggests co-located emission regions in the outer magnetosphere.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enPSR B1957+20)
dc.subject.enradiation mechanisms: non-thermal
dc.subject.engamma rays: general
dc.subject.enpulsars: general
dc.subject.enpulsars: individual (PSR B1937+21
dc.title.enPulsed Gamma Rays from the Original Millisecond and Black Widow Pulsars: a case for Caustic Radio Emission?
dc.typeArticle de revue
dc.identifier.doi10.1088/0004-637X/744/1/33
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.subject.halPhysique [physics]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1110.1271
bordeaux.journalThe Astrophysical Journal
bordeaux.page33
bordeaux.volume744
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierin2p3-00664205
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00664205v1
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