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Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
dc.contributor.author | J. PLETSCH, H. | |
dc.contributor.author | GUILLEMOT, L. | |
dc.contributor.author | FEHRMANN, H. | |
dc.contributor.author | ALLEN, B. | |
dc.contributor.author | KRAMER, M. | |
dc.contributor.author | AULBERT, C. | |
dc.contributor.author | ACKERMANN, Markus | |
dc.contributor.author | AJELLO, Marco | |
dc.contributor.author | DE ANGELIS, A. | |
dc.contributor.author | B. ATWOOD, W. | |
dc.contributor.author | BALDINI, Luca | |
dc.contributor.author | BALLET11, J. | |
dc.contributor.author | BARBIELLINI, Guido | |
dc.contributor.author | BASTIERI, D. | |
dc.contributor.author | BECHTOL, K. | |
dc.contributor.author | BELLAZZINI, R. | |
dc.contributor.author | W. BORGLAND, A. | |
dc.contributor.author | BOTTACINI, E. | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | J. BRANDT, T. | |
dc.contributor.author | BREGEON, J. | |
dc.contributor.author | BRIGIDA, M. | |
dc.contributor.author | BUEHLER, R. | |
dc.contributor.author | BUSON, S. | |
dc.contributor.author | A. CALIANDRO, G. | |
dc.contributor.author | A. CAMERON, R. | |
dc.contributor.author | CARAVEO, P. A. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | M. CASANDJIAN, J. | |
dc.contributor.author | CECCHI, C. | |
dc.contributor.author | ÇELIK, Ö. | |
hal.structure.identifier | Commonwealth Scientific and Industrial Research Organisation [Canberra] [CSIRO] | |
dc.contributor.author | CHARLES, E. | |
dc.contributor.author | C. G. CHAVES, R. | |
dc.contributor.author | C. CHEUNG, C. | |
dc.contributor.author | CHIANG, J. | |
dc.contributor.author | CIPRINI, S. | |
dc.contributor.author | CLAUS, R. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | COHEN-TANUGI, J. | |
dc.contributor.author | CONRAD, J. | |
dc.contributor.author | CUTINI, S. | |
dc.contributor.author | D'AMMANDO, F. | |
dc.contributor.author | D. DERMER, C. | |
dc.contributor.author | W. DIGEL, S. | |
dc.contributor.author | S. DRELL, P. | |
dc.contributor.author | DRLICA-WAGNER, A. | |
dc.contributor.author | DUBOIS, R. | |
hal.structure.identifier | GLAST | |
dc.contributor.author | DUMORA, D. | |
dc.contributor.author | FAVUZZI, C. | |
dc.contributor.author | C. FERRARA, E. | |
dc.contributor.author | FRANCKOWIAK, A. | |
dc.contributor.author | FUKAZAWA, Y. | |
dc.contributor.author | FUSCO, P. | |
dc.contributor.author | GARDANO, F. | |
dc.contributor.author | GEHRELS, N. | |
dc.contributor.author | GERMANI, S. | |
dc.contributor.author | GIGLIETTO, N. | |
dc.contributor.author | GIORDANO, F. | |
dc.contributor.author | GIROLETTI, M. | |
dc.contributor.author | GODFREY, G. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | A. GRENIER, I. | |
dc.contributor.author | GRONDIN, M.-H. | |
dc.contributor.author | E. GROVE, J. | |
dc.contributor.author | GUIRIEC, S. | |
dc.contributor.author | HADASCH, D. | |
dc.contributor.author | HANABATA, Y. | |
dc.contributor.author | K. HARDING, A. | |
dc.contributor.author | R. DEN HARTOG, P. | |
dc.contributor.author | HAYASHIDA, M. | |
dc.contributor.author | HAYS, E. | |
dc.contributor.author | B. HILL7, A. | |
hal.structure.identifier | GLAST | |
dc.contributor.author | HOU, X. | |
dc.contributor.author | E. HUGHES, R. | |
dc.contributor.author | JÓHANNESSON, G. | |
dc.contributor.author | S. JACKSON, M. | |
dc.contributor.author | JOGLER, T. | |
dc.contributor.author | S. JOHNSON, A. | |
dc.contributor.author | N. JOHNSON, W. | |
dc.contributor.author | KATAOKA, J. | |
dc.contributor.author | KERR, M. | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | KNÖDLSEDER, Jürgen | |
dc.contributor.author | KUSS, M. | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | LANDE, J. | |
dc.contributor.author | LARSSON, S. | |
dc.contributor.author | LATRONICO, L. | |
hal.structure.identifier | GLAST | |
dc.contributor.author | LEMOINE-GOUMARD, M. | |
dc.contributor.author | LONGO, F. | |
dc.contributor.author | LOPARCO, F. | |
dc.contributor.author | N. LOVELLETTE, M. | |
dc.contributor.author | LUBRANO, P. | |
dc.contributor.author | MASSARO, F. | |
dc.contributor.author | MAYER, M. | |
dc.contributor.author | N. MAZZIOTTA, M. | |
dc.contributor.author | E. MCENERY, J. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | MEHAULT, J. | |
dc.contributor.author | F. MICHELSON, P. | |
dc.contributor.author | MITTHUMSIRI, W. | |
dc.contributor.author | MIZUNO, T. | |
dc.contributor.author | E. MONZANI, M. | |
dc.contributor.author | MORSELLI, A. | |
dc.contributor.author | V. MOSKALENKO, I. | |
dc.contributor.author | MURGIA, S. | |
dc.contributor.author | NAKAMORI, T. | |
dc.contributor.author | NEMMEN, R. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | NUSS, E. | |
dc.contributor.author | OHNO, M. | |
dc.contributor.author | OHSUGI, T. | |
dc.contributor.author | OMODEI, N. | |
dc.contributor.author | ORIENTI, M. | |
dc.contributor.author | ORLANDO, E. | |
dc.contributor.author | DE PALMA, F. | |
dc.contributor.author | PANEQUE, D. | |
dc.contributor.author | S. PERKINS, J. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | PIRON, F. | |
dc.contributor.author | PIVATO, G. | |
dc.contributor.author | PORTER, T.A. | |
dc.contributor.author | RAINÒ, S. | |
dc.contributor.author | RANDO, R. | |
dc.contributor.author | S. RAY, P. | |
dc.contributor.author | RAZZANO, M. | |
dc.contributor.author | REIMER, A. | |
dc.contributor.author | REIMER, O. | |
hal.structure.identifier | GLAST | |
dc.contributor.author | REPOSEUR, T. | |
dc.contributor.author | RITZ, S. | |
dc.contributor.author | W. ROMANI, R. | |
dc.contributor.author | ROMOLI, C. | |
dc.contributor.author | SANCHEZ, D.A. | |
dc.contributor.author | M. SAZ PARKINSON, P. | |
dc.contributor.author | SCHULZ, A. | |
dc.contributor.author | SGRÒ1, C. | |
dc.contributor.author | DO COUTO E SILVA, E. | |
dc.contributor.author | J. SISKIND, E. | |
hal.structure.identifier | GLAST | |
dc.contributor.author | SMITH, David Stanley | |
dc.contributor.author | SPANDRE, G. | |
dc.contributor.author | SPINELLI, P. | |
dc.contributor.author | J. SUSON, D. | |
dc.contributor.author | TAKAHASHI, H. | |
dc.contributor.author | TANAKA, T. | |
dc.contributor.author | B. THAYER, J. | |
dc.contributor.author | G. THAYER, J. | |
dc.contributor.author | J. THOMPSON, D. | |
dc.contributor.author | TIBALDO, L. | |
dc.contributor.author | TINIVELLA, M. | |
dc.contributor.author | TROJA, E. | |
dc.contributor.author | L. USHER, T. | |
dc.contributor.author | VANDENBROUCKE, J. | |
hal.structure.identifier | Laboratoire Univers et Particules de Montpellier [LUPM] | |
dc.contributor.author | VASILEIOU, V. | |
dc.contributor.author | VIANELLO, G. | |
dc.contributor.author | VITALE, V. | |
dc.contributor.author | P. WAITE, A. | |
dc.contributor.author | L. WINER, B. | |
dc.contributor.author | S. WOOD, K. | |
dc.contributor.author | WOOD, M. | |
dc.contributor.author | YANG, Z. | |
dc.contributor.author | ZIMMER, S. | |
dc.date.issued | 2012-10-25 | |
dc.identifier.issn | 0036-8075 | |
dc.description.abstractEn | Millisecond pulsars, old neutron stars spun up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311−3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found. | |
dc.language.iso | en | |
dc.publisher | American Association for the Advancement of Science (AAAS) | |
dc.title.en | Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1126/science.1229054 | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE] | |
dc.identifier.arxiv | 1211.1385 | |
bordeaux.journal | Science | |
bordeaux.page | 1314-1317 | |
bordeaux.volume | 338 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00769556 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00769556v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Science&rft.date=2012-10-25&rft.volume=338&rft.spage=1314-1317&rft.epage=1314-1317&rft.eissn=0036-8075&rft.issn=0036-8075&rft.au=J.%20PLETSCH,%20H.&GUILLEMOT,%20L.&FEHRMANN,%20H.&ALLEN,%20B.&KRAMER,%20M.&rft.genre=article |
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