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Radio and Gamma-Ray Constraints on the Emission Geometry and Birthplace of PSR J2043+2740

dc.contributor.authorNOUTSOS, A.
dc.contributor.authorABDO, A.A.
dc.contributor.authorACKERMANN, Markus
dc.contributor.authorAJELLO, Marco
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorBALLET, Jean
dc.contributor.authorBARBIELLINI, Guido
dc.contributor.authorBARING, Matthew G.
dc.contributor.authorBASTIERI, D.
dc.contributor.authorBECHTOL, K.
dc.contributor.authorBELLAZZINI, R.
dc.contributor.authorBERENJI, B.
dc.contributor.authorBONAMENTE, E.
dc.contributor.authorBORGLAND, A. W.
dc.contributor.authorBREGEON, J.
dc.contributor.authorBREZ, A.
dc.contributor.authorBRIGIDA, M.
hal.structure.identifierLaboratoire Leprince-Ringuet [LLR]
dc.contributor.authorBRUEL, Pascal
dc.contributor.authorBUEHLER, R.
dc.contributor.authorBUSETTO, G.
dc.contributor.authorCALIANDRO, G. A.
dc.contributor.authorCAMERON, R. A.
dc.contributor.authorCAMILO, F.
dc.contributor.authorCARAVEO, P. A.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorCASANDJIAN, J. M.
dc.contributor.authorCECCHI, C.
dc.contributor.authorCELIK, O.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorCHATY, S.
dc.contributor.authorCHEKHTMAN, A.
dc.contributor.authorCHIANG, J.
dc.contributor.authorCIPRINI, S.
dc.contributor.authorCLAUS, R.
hal.structure.identifierLaboratoire de physique et chimie de l'environnement [LPCE]
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
dc.contributor.authorCOGNARD, Ismaël
hal.structure.identifierLaboratoire de Physique Théorique et Astroparticules [LPTA]
dc.contributor.authorCOHEN-TANUGI, J.
dc.contributor.authorCOLAFRANCESCO, S.
dc.contributor.authorCUTINI, S.
dc.contributor.authorDERMER, C. D.
dc.contributor.authorDE PALMA, F.
dc.contributor.authorDRELL, P. S.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorDUMORA, D.
dc.contributor.authorESPINOZA, C. M.
dc.contributor.authorFAVUZZI, C.
dc.contributor.authorFERRARA, E. C.
dc.contributor.authorFOCKE, W. B.
dc.contributor.authorFRAILIS, M.
dc.contributor.authorFREIRE, P. C. C.
dc.contributor.authorFUKAZAWA, Y.
dc.contributor.authorFUNK, S.
dc.contributor.authorFUSCO, P.
dc.contributor.authorGARGANO, F.
dc.contributor.authorGERMANI, S.
dc.contributor.authorGIGLIETTO, N.
dc.contributor.authorGIORDANO, F.
dc.contributor.authorGIROLETTI, M.
dc.contributor.authorGODFREY, G.
dc.contributor.authorGRANDI, P.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorGRENIER, I. A.
dc.contributor.authorGROVE, J. E.
dc.contributor.authorGUILLEMOT, L.
dc.contributor.authorGUIRIEC, S.
dc.contributor.authorHARDING, A. K.
dc.contributor.authorHUGHES, R. E.
dc.contributor.authorJACKSON, M. S.
dc.contributor.authorJOHANNESSON, G.
dc.contributor.authorJOHNSON, A. S.
dc.contributor.authorJOHNSON, T. J.
dc.contributor.authorJOHNSON, W. N.
dc.contributor.authorJOHNSTON, S.
dc.contributor.authorKAMAE, T.
dc.contributor.authorKATAGIRI, H.
dc.contributor.authorKATAOKA, J.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorKNÖDLSEDER, Jürgen
dc.contributor.authorKRAMER, M.
dc.contributor.authorKUSS, M.
dc.contributor.authorLANDE, J.
dc.contributor.authorLEE, S. -H.
dc.contributor.authorLONGO, F.
dc.contributor.authorLOPARCO, F.
dc.contributor.authorLOVELLETTE, M. N.
dc.contributor.authorLUBRANO, P.
dc.contributor.authorLYNE, A. G.
dc.contributor.authorMAKEEV, A.
dc.contributor.authorMARELLI, M.
dc.contributor.authorMAZZIOTTA, M. N.
dc.contributor.authorMCENERY, J. E.
hal.structure.identifierLaboratoire de Physique Théorique et Astroparticules [LPTA]
dc.contributor.authorMEHAULT, J.
dc.contributor.authorMICHELSON, P. F.
dc.contributor.authorMIZUNO, T.
dc.contributor.authorMONTE, C.
dc.contributor.authorMONZANI, M. E.
dc.contributor.authorMORSELLI, A.
dc.contributor.authorMOSKALENKO, I. V.
dc.contributor.authorMURGIA, S.
dc.contributor.authorNAUMANN-GODO, M.
dc.contributor.authorNOLAN, P. L.
hal.structure.identifierLaboratoire de Physique Théorique et Astroparticules [LPTA]
dc.contributor.authorNUSS, E.
dc.contributor.authorOHSUGI, T.
dc.contributor.authorOKUMURA, A.
dc.contributor.authorOMODEI, N.
dc.contributor.authorORLANDO, E.
dc.contributor.authorORMES, J. F.
dc.contributor.authorPANETTA, J. H.
dc.contributor.authorPARENT, D.
hal.structure.identifierLaboratoire de Physique Théorique et Astroparticules [LPTA]
dc.contributor.authorPELASSA, V.
dc.contributor.authorPEPE, M.
dc.contributor.authorPERSIC, M.
dc.contributor.authorPESCE-ROLLINS, M.
hal.structure.identifierLaboratoire de Physique Théorique et Astroparticules [LPTA]
dc.contributor.authorPIRON, F.
dc.contributor.authorPORTER, T. A.
dc.contributor.authorRAIN, S.
dc.contributor.authorRAY, P. S.
dc.contributor.authorRAZZANO, M.
dc.contributor.authorREIMER, A.
dc.contributor.authorREIMER, O.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorREPOSEUR, T.
dc.contributor.authorROMANI, R. W.
dc.contributor.authorSADROZINSKI, H. F. -W.
dc.contributor.authorSANDER, A.
dc.contributor.authorPARKINSON, P. M. Saz
dc.contributor.authorSGRO, C.
dc.contributor.authorSISKIND, E. J.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorSMITH, D. A.
dc.contributor.authorSMITH, P. D.
dc.contributor.authorSPANDRE, G.
dc.contributor.authorSPINELLI, P.
dc.contributor.authorSTAPPERS, B. W.
dc.contributor.authorSTRICKMAN, M. S.
dc.contributor.authorSUSON, D. J.
dc.contributor.authorTAKAHASHI, H.
dc.contributor.authorTANAKA, T.
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
hal.structure.identifierLaboratoire de physique et chimie de l'environnement [LPCE]
dc.contributor.authorTHEUREAU, Gilles
dc.contributor.authorTHOMPSON, D. J.
dc.contributor.authorTHORSETT, S. E.
dc.contributor.authorTIBOLLA, O.
dc.contributor.authorTORRES, D. F.
dc.contributor.authorTRAMACERE, A.
dc.contributor.authorUSHER, T. L.
dc.contributor.authorVANDENBROUCKE, J.
dc.contributor.authorVIANELLO, G.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorVILCHEZ, N.
dc.contributor.authorVILLATA, M.
dc.contributor.authorVITALE, V.
dc.contributor.authorVON KIENLIN, A.
dc.contributor.authorWAITE, A. P.
dc.contributor.authorWANG, P.
dc.contributor.authorWATTERS, K.
dc.contributor.authorWELTEVREDE, P.
dc.contributor.authorWINER, B. L.
dc.contributor.authorWOOD, K. S.
dc.contributor.authorZIEGLER, M.
dc.date.issued2011-02-20
dc.identifier.issn0004-637X
dc.description.abstractEnWe report on the first year of Fermi gamma-ray observations of pulsed high-energy emission from the old PSR J2043+2740. The study of the gamma-ray efficiency of such old pulsars gives us an insight into the evolution of pulsars' ability to emit in gammma rays as they age. The gamma-ray lightcurve of this pulsar above 0.1 GeV is clearly defined by two sharp peaks, 0.353+/-0.035 periods apart. We have combined the gamma-ray profile characteristics of PSR J2043+2740 with the geometrical properties of the pulsar's radio emission, derived from radio polarization data, and constrained the pulsar-beam geometry in the framework of a Two Pole Caustic and an Outer Gap model. The ranges of magnetic inclination and viewing angle were determined to be {alpha,zeta}~{52-57,61-68} for the Two Pole Caustic model, and {alpha,zeta}~{62-73,74-81} and {alpha,zeta}~{72-83,60-75} for the Outer Gap model. Based on this geometry, we assess possible birth locations for this pulsar and derive a likely proper motion, sufficiently high to be measurable with VLBI. At a characteristic age of 1.2 Myr, PSR J2043+2740 is the third oldest of all discovered, non-recycled, gamma-ray pulsars: it is twice as old as the next oldest, PSR J0357+32, and younger only than the recently discovered PSR J1836+5925 and PSR J2055+25, both of which are at least 5 and 10 times less energetic, respectively.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enpulsars: individual (PSR J2043 + 2740)
dc.subject.engamma rays: stars
dc.title.enRadio and Gamma-Ray Constraints on the Emission Geometry and Birthplace of PSR J2043+2740
dc.typeArticle de revue
dc.identifier.doi10.1088/0004-637X/728/2/77
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.identifier.arxiv1012.4658
bordeaux.journalThe Astrophysical Journal
bordeaux.page77
bordeaux.volume728
bordeaux.peerReviewedoui
hal.identifierin2p3-00586586
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00586586v1
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