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Article: Fermi detection of a luminous γ-ray pulsar in a globular cluster

TitleFermi detection of a luminous γ-ray pulsar in a globular cluster
Authors
Freire, PCCAbdo, AAAjello, MAllafort, ABallet, JBarbiellini, GBastieri, DBechtol, KBellazzini, RBlandford, RDBloom, EDOkumura, AOmodei, NOrlando, EOzaki, MPaneque, DParent, DPesceRollins, MPierbattista, MPiron, FPorter, TABonamente, ERainò, SRansom, SMRay, PSReimer, AReimer, OReposeur, TRitz, SRomani, RWRoth, MSadrozinski, HFWBorgland, AWSaz Parkinson, PMSgrò, CShannon, RSiskind, EJSmith, DASmith, PDSpinelli, PStappers, BWSuson, DJTakahashi, HBrigida, MTanaka, TTauris, TMThayer, JBTheureau, GThompson, DJThorsett, SETibaldo, LTorres, DFTosti, GTroja, EBruel, PVandenbroucke, JVan Etten, AVasileiou, VVenter, CVianello, GVilchez, NVitale, VWaite, APWang, PWood, KSBuehler, RYang, ZZiegler, MZimmer, SBuson, SCaliandro, GACameron, RACamilo, FCaraveo, PACecchi, CÇelik, ÖCharles, EChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCognard, ICohenTanugi, JCominsky, LRDe Palma, FDermer, CDDo Couto E Silva, EDormody, MDrell, PSDubois, RDumora, DEspinoza, CMFavuzzi, CFegan, SJFerrara, ECFocke, WBFortin, PFukazawa, YFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiglietto, NGiordano, FGiroletti, MGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHadasch, DHarding, AKJóhannesson, GJohnson, ASJohnson, TJJohnston, SKatagiri, HKataoka, JKeith, MKerr, MKnödlseder, JKramer, MKuss, MLande, JLatronico, LLee, SHLemoineGoumard, MLongo, FLoparco, FLovellette, MNLubrano, PLyne, AGManchester, RNMarelli, MMazziotta, MNMcenery, JEMichelson, PFMizuno, TMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNakamori, TNolan, PLNorris, JPNuss, EOhsugi, T
Issue Date2011
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2011, v. 334 n. 6059, p. 1107-1110 How to Cite?
AbstractWe report on the Fermi Large Area Telescope's detection of γ-ray (>100 mega-electron volts) pulsations from pulsar J1823-3021A in the globular cluster NGC 6624 with high significance (∼7 σ). Its γ-ray luminosity, Lγ = (8.4 ± 1.6) × 1034 ergs per second, is the highest observed for any millisecond pulsar (MSP) to date, and it accounts for most of the cluster emission. The nondetection of the cluster in the off-pulse phase implies that it contains <32 γ-ray MSPs, not ∼100 as previously estimated. The γ-ray luminosity indicates that the unusually large rate of change of its period is caused by its intrinsic spin-down. This implies that J1823-3021A has the largest magnetic field and is the youngest MSP ever detected and that such anomalous objects might be forming at rates comparable to those of the more normal MSPs.
Persistent Identifierhttp://hdl.handle.net/10722/188412
ISSN
2015 Impact Factor: 34.661
2015 SCImago Journal Rankings: 13.217
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorFreire, PCCen_US
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAllafort, Aen_US
dc.contributor.authorBallet, Jen_US
dc.contributor.authorBarbiellini, Gen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorBechtol, Ken_US
dc.contributor.authorBellazzini, Ren_US
dc.contributor.authorBlandford, RDen_US
dc.contributor.authorBloom, EDen_US
dc.contributor.authorOkumura, Aen_US
dc.contributor.authorOmodei, Nen_US
dc.contributor.authorOrlando, Een_US
dc.contributor.authorOzaki, Men_US
dc.contributor.authorPaneque, Den_US
dc.contributor.authorParent, Den_US
dc.contributor.authorPesceRollins, Men_US
dc.contributor.authorPierbattista, Men_US
dc.contributor.authorPiron, Fen_US
dc.contributor.authorPorter, TAen_US
dc.contributor.authorBonamente, Een_US
dc.contributor.authorRainò, Sen_US
dc.contributor.authorRansom, SMen_US
dc.contributor.authorRay, PSen_US
dc.contributor.authorReimer, Aen_US
dc.contributor.authorReimer, Oen_US
dc.contributor.authorReposeur, Ten_US
dc.contributor.authorRitz, Sen_US
dc.contributor.authorRomani, RWen_US
dc.contributor.authorRoth, Men_US
dc.contributor.authorSadrozinski, HFWen_US
dc.contributor.authorBorgland, AWen_US
dc.contributor.authorSaz Parkinson, PMen_US
dc.contributor.authorSgrò, Cen_US
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dc.contributor.authorBuehler, Ren_US
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dc.contributor.authorDrell, PSen_US
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dc.contributor.authorKuss, Men_US
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dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLovellette, MNen_US
dc.contributor.authorLubrano, Pen_US
dc.contributor.authorLyne, AGen_US
dc.contributor.authorManchester, RNen_US
dc.contributor.authorMarelli, Men_US
dc.contributor.authorMazziotta, MNen_US
dc.contributor.authorMcenery, JEen_US
dc.contributor.authorMichelson, PFen_US
dc.contributor.authorMizuno, Ten_US
dc.contributor.authorMoiseev, AAen_US
dc.contributor.authorMonte, Cen_US
dc.contributor.authorMonzani, MEen_US
dc.contributor.authorMorselli, Aen_US
dc.contributor.authorMoskalenko, IVen_US
dc.contributor.authorMurgia, Sen_US
dc.contributor.authorNakamori, Ten_US
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dc.date.accessioned2013-09-03T04:05:38Z-
dc.date.available2013-09-03T04:05:38Z-
dc.date.issued2011en_US
dc.identifier.citationScience, 2011, v. 334 n. 6059, p. 1107-1110en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188412-
dc.description.abstractWe report on the Fermi Large Area Telescope's detection of γ-ray (>100 mega-electron volts) pulsations from pulsar J1823-3021A in the globular cluster NGC 6624 with high significance (∼7 σ). Its γ-ray luminosity, Lγ = (8.4 ± 1.6) × 1034 ergs per second, is the highest observed for any millisecond pulsar (MSP) to date, and it accounts for most of the cluster emission. The nondetection of the cluster in the off-pulse phase implies that it contains <32 γ-ray MSPs, not ∼100 as previously estimated. The γ-ray luminosity indicates that the unusually large rate of change of its period is caused by its intrinsic spin-down. This implies that J1823-3021A has the largest magnetic field and is the youngest MSP ever detected and that such anomalous objects might be forming at rates comparable to those of the more normal MSPs.en_US
dc.languageengen_US
dc.publisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.orgen_US
dc.relation.ispartofScienceen_US
dc.titleFermi detection of a luminous γ-ray pulsar in a globular clusteren_US
dc.typeArticleen_US
dc.identifier.emailVan Etten, A: pablosp@hku.hken_US
dc.identifier.authorityVan Etten, A=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1126/science.1207141en_US
dc.identifier.scopuseid_2-s2.0-82255179077en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-82255179077&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume334en_US
dc.identifier.issue6059en_US
dc.identifier.spage1107en_US
dc.identifier.epage1110en_US
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