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Article: A population of gamma-ray millisecond pulsars seen with the fermi large area telescope

TitleA population of gamma-ray millisecond pulsars seen with the fermi large area telescope
Authors
Abdo, AAAckermann, MAjello, MAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBaring, MGBastieri, DBaughman, BMLande, JLatronico, LLemoineGoumard, MLongo, FLoparco, FLott, BLovellette, MNLubrano, PMadejski, GMMakeev, ABechtol, KManchester, RNMarelli, MMazziotta, MNMcconville, WMcenery, JEMclaughlin, MAMeurer, CMichelson, PFMitthumsiri, WMizuno, TBellazzini, RMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNolan, PLNorris, JPNuss, EOhsugi, TBerenji, BOmodei, NOrlando, EOrmes, JFPaneque, DPanetta, JHParent, DPelassa, VPepe, MPesceRollins, MPiron, FBignami, GFPorter, TARainò, SRando, RRansom, SMRay, PSRazzano, MRea, NReimer, AReimer, OReposeur, TBlandford, RDRitz, SRochester, LSRodriguez, AYRomani, RWRoth, MRyde, FSadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMBloom, EDScargle, JDSchalk, TLSgrò, CSiskind, EJSmith, DASmith, PDSpandre, GSpinelli, PStappers, BWStarck, JLBonamente, EStriani, EStrickman, MSSuson, DJTajima, HTakahashi, HTanaka, TThayer, JBThayer, JGTheureau, GThompson, DJBorgland, AWThorsett, SETibaldo, LTorres, DFTosti, GTramacere, AUchiyama, YUsher, TLVan Etten, AVasileiou, VVenter, CBregeon, JVilchez, NVitale, VWaite, APWallace, EWang, PWatters, KWebb, NWeltevrede, PWiner, BLWood, KSBrez, AYlinen, TZiegler, MBrigida, MBruel, PBurnett, THCaliandro, GACameron, RACamilo, FCaraveo, PACarlson, PCasandjian, JMCecchi, CÇelik, ÖCharles, EChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCognard, ICohenTanugi, JCominsky, LRConrad, JCorbet, RCutini, SDermer, CDDesvignes, GDe Angelis, ADe Luca, ADe Palma, FDigel, SWDormody, MDo Couto E Silva, EDrell, PSDubois, RDumora, DEdmonds, YFarnier, CFavuzzi, CFegan, SJFocke, WBFrailis, MFreire, PCCFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiebels, BGiglietto, NGiordano, FGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHayashida, MHays, EHobbs, GHughes, REJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNJohnston, SKamae, TKatagiri, HKataoka, JKawai, NKerr, MKnödlseder, JKocian, MLKramer, MKuss, M
Issue Date2009
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2009, v. 325 n. 5942, p. 848-852 How to Cite?
DOI: http://dx.doi.org/10.1126/science.1176113
AbstractPulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to millisecond periods and begin radiating again. We searched Fermi Large Area Telescope data for pulsations from all known millisecond pulsars (MSPs) outside of globular clusters, using rotation parameters from radio telescopes. Strong gamma-ray pulsations were detected for eight MSPs. The gamma-ray pulse profiles and spectral properties resemble those of young gamma-ray pulsars. The basic emission mechanism seems to be the same for MSPs and young pulsars, with the emission originating in regions far from the neutron star surface.
Persistent Identifierhttp://hdl.handle.net/10722/188367
ISSN
0036-8075
2023 Impact Factor: 44.7
2023 SCImago Journal Rankings: 11.902
ISI Accession Number ID
WOS:000269242400039
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAtwood, WBen_US
dc.contributor.authorAxelsson, Men_US
dc.contributor.authorBaldini, Len_US
dc.contributor.authorBallet, Jen_US
dc.contributor.authorBarbiellini, Gen_US
dc.contributor.authorBaring, MGen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorBaughman, BMen_US
dc.contributor.authorLande, Jen_US
dc.contributor.authorLatronico, Len_US
dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLott, Ben_US
dc.contributor.authorLovellette, MNen_US
dc.contributor.authorLubrano, Pen_US
dc.contributor.authorMadejski, GMen_US
dc.contributor.authorMakeev, Aen_US
dc.contributor.authorBechtol, Ken_US
dc.contributor.authorManchester, RNen_US
dc.contributor.authorMarelli, Men_US
dc.contributor.authorMazziotta, MNen_US
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dc.contributor.authorMcenery, JEen_US
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dc.contributor.authorMitthumsiri, Wen_US
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dc.contributor.authorPepe, Men_US
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dc.contributor.authorWang, Pen_US
dc.contributor.authorWatters, Ken_US
dc.contributor.authorWebb, Nen_US
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dc.contributor.authorWiner, BLen_US
dc.contributor.authorWood, KSen_US
dc.contributor.authorBrez, Aen_US
dc.contributor.authorYlinen, Ten_US
dc.contributor.authorZiegler, Men_US
dc.contributor.authorBrigida, Men_US
dc.contributor.authorBruel, Pen_US
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dc.contributor.authorCaliandro, GAen_US
dc.contributor.authorCameron, RAen_US
dc.contributor.authorCamilo, Fen_US
dc.contributor.authorCaraveo, PAen_US
dc.contributor.authorCarlson, Pen_US
dc.contributor.authorCasandjian, JMen_US
dc.contributor.authorCecchi, Cen_US
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dc.contributor.authorCharles, Een_US
dc.contributor.authorChekhtman, Aen_US
dc.contributor.authorCheung, CCen_US
dc.contributor.authorChiang, Jen_US
dc.contributor.authorCiprini, Sen_US
dc.contributor.authorClaus, Ren_US
dc.contributor.authorCognard, Ien_US
dc.contributor.authorCohenTanugi, Jen_US
dc.contributor.authorCominsky, LRen_US
dc.contributor.authorConrad, Jen_US
dc.contributor.authorCorbet, Ren_US
dc.contributor.authorCutini, Sen_US
dc.contributor.authorDermer, CDen_US
dc.contributor.authorDesvignes, Gen_US
dc.contributor.authorDe Angelis, Aen_US
dc.contributor.authorDe Luca, Aen_US
dc.contributor.authorDe Palma, Fen_US
dc.contributor.authorDigel, SWen_US
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dc.contributor.authorGehrels, Nen_US
dc.contributor.authorGermani, Sen_US
dc.contributor.authorGiebels, Ben_US
dc.contributor.authorGiglietto, Nen_US
dc.contributor.authorGiordano, Fen_US
dc.contributor.authorGlanzman, Ten_US
dc.contributor.authorGodfrey, Gen_US
dc.contributor.authorGrenier, IAen_US
dc.contributor.authorGrondin, MHen_US
dc.contributor.authorGrove, JEen_US
dc.contributor.authorGuillemot, Len_US
dc.contributor.authorGuiriec, Sen_US
dc.contributor.authorHanabata, Yen_US
dc.contributor.authorHarding, AKen_US
dc.contributor.authorHayashida, Men_US
dc.contributor.authorHays, Een_US
dc.contributor.authorHobbs, Gen_US
dc.contributor.authorHughes, REen_US
dc.contributor.authorJóhannesson, Gen_US
dc.contributor.authorJohnson, ASen_US
dc.contributor.authorJohnson, RPen_US
dc.contributor.authorJohnson, TJen_US
dc.contributor.authorJohnson, WNen_US
dc.contributor.authorJohnston, Sen_US
dc.contributor.authorKamae, Ten_US
dc.contributor.authorKatagiri, Hen_US
dc.contributor.authorKataoka, Jen_US
dc.contributor.authorKawai, Nen_US
dc.contributor.authorKerr, Men_US
dc.contributor.authorKnödlseder, Jen_US
dc.contributor.authorKocian, MLen_US
dc.contributor.authorKramer, Men_US
dc.contributor.authorKuss, Men_US
dc.date.accessioned2013-09-03T04:03:59Z-
dc.date.available2013-09-03T04:03:59Z-
dc.date.issued2009en_US
dc.identifier.citationScience, 2009, v. 325 n. 5942, p. 848-852en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188367-
dc.description.abstractPulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to millisecond periods and begin radiating again. We searched Fermi Large Area Telescope data for pulsations from all known millisecond pulsars (MSPs) outside of globular clusters, using rotation parameters from radio telescopes. Strong gamma-ray pulsations were detected for eight MSPs. The gamma-ray pulse profiles and spectral properties resemble those of young gamma-ray pulsars. The basic emission mechanism seems to be the same for MSPs and young pulsars, with the emission originating in regions far from the neutron star surface.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.titleA population of gamma-ray millisecond pulsars seen with the fermi large area telescopeen_US
dc.typeArticleen_US
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, PM=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1126/science.1176113en_US
dc.identifier.pmid19574349-
dc.identifier.scopuseid_2-s2.0-68949213844en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-68949213844&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume325en_US
dc.identifier.issue5942en_US
dc.identifier.spage848en_US
dc.identifier.epage852en_US
dc.identifier.isiWOS:000269242400039-
dc.publisher.placeUnited Statesen_US
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dc.identifier.issnl0036-8075-

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