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Six millisecond pulsars detected by the Fermi Large Area Telescope and the radio/gamma-ray connection of millisecond pulsars

dc.contributor.authorESPINOZA, C.M.
dc.contributor.authorGUILLEMOT, Lucas
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorCELIK, O.
hal.structure.identifierJodrell Bank Centre for Astrophysics
dc.contributor.authorWELTEVREDE, P.
hal.structure.identifierJodrell Bank Centre for Astrophysics
dc.contributor.authorSTAPPERS, B.W.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorSMITH, D.A.
dc.contributor.authorKERR, M.
dc.contributor.authorE. ZAVLIN, V.
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.authorCOGNARD, Ismaël
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorEATOUGH, R. P.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorFREIRE, P. C. C.
hal.structure.identifierJodrell Bank Centre for Astrophysics
dc.contributor.authorJANSSEN, G. H.
hal.structure.identifierArecibo Observatory, National Astronomy and Ionosphere Center [NAIC]
dc.contributor.authorCAMILO, F.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
hal.structure.identifierUnité Scientifique de la Station de Nançay [USN]
dc.contributor.authorDESVIGNES, Grégory
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorHOU, X.
hal.structure.identifierLos Alamos National Laboratory [LANL]
dc.contributor.authorJOHNSTON, S.
hal.structure.identifierCSIRO Astronomy and Space Science
dc.contributor.authorKEITH, M.
hal.structure.identifierJodrell Bank Centre for Astrophysics
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorKRAMER, M.
dc.contributor.authorLYNE, A.
hal.structure.identifierCSIRO Astronomy and Space Science
dc.contributor.authorMANCHESTER, R. N.
hal.structure.identifierNational Radio Astronomy Observatory [Green Bank] [NRAO]
dc.contributor.authorRANSOM, S.M.
hal.structure.identifierNASA Marshall Space Flight Center [MSFC]
dc.contributor.authorRAY, P.S.
hal.structure.identifierCSIRO Astronomy and Space Science
dc.contributor.authorSHANNON, R.
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
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorWEBB, N.
dc.date.issued2013
dc.identifier.issn0035-8711
dc.description.abstractEnWe report on the discovery of gamma-ray pulsations from five millisecond pulsars (MSPs) using the Fermi Large Area Telescope (LAT) and timing ephemerides provided by various radio observatories. We also present confirmation of the gamma-ray pulsations from a sixth source, PSR J2051−0827. Five of these six MSPs are in binary systems: PSRs J1713+0747, J1741+1351, J1600−3053 and the two black widow binary pulsars PSRs J0610−2100 and J2051−0827. The only isolated MSP is the nearby PSR J1024−0719, which is also known to emit X-rays. We present X-ray observations in the direction of PSRs J1600−3053 and J2051−0827. While PSR J2051−0827 is firmly detected, we can only give upper limits for the X-ray flux of PSR J1600−3053. There are no dedicated X-ray observations available for the other three objects. The MSPs mentioned above, together with most of the MSPs detected by Fermi, are used to put together a sample of 30 gamma-ray MSPs. This sample is used to study the morphology and phase connection of radio and gamma-ray pulse profiles. We show that MSPs with pulsed gamma-ray emission which is phase-aligned with the radio emission present the steepest radio spectra and the largest magnetic fields at the light cylinder among all MSPs. Also, we observe a trend towards very low, or undetectable, radio linear polarization levels. These properties
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.title.enSix millisecond pulsars detected by the Fermi Large Area Telescope and the radio/gamma-ray connection of millisecond pulsars
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/sts657
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.identifier.arxiv1212.4360
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page571 - 587
bordeaux.volume430
bordeaux.peerReviewedoui
hal.identifierin2p3-00833913
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00833913v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society&rft.date=2013&rft.volume=430&rft.spage=571%20-%20587&rft.epage=571%20-%20587&rft.eissn=0035-8711&rft.issn=0035-8711&rft.au=ESPINOZA,%20C.M.&GUILLEMOT,%20Lucas&CELIK,%20O.&WELTEVREDE,%20P.&STAPPERS,%20B.W.&rft.genre=article


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