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Article: Detection of high-energy gamma-ray emission from the globular cluster 47 tucanae with Fermi

TitleDetection of high-energy gamma-ray emission from the globular cluster 47 tucanae with Fermi
Authors
Abdo, AAAckermann, MAjello, MAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNolan, PLNorris, JPNuss, EOhsugi, TBellazzini, ROmodei, NOrlando, EOrmes, JFPaneque, DPanetta, JHParent, DPelassa, VPepe, MPierbattista, MPiron, FBerenji, BPorter, TARainò, SRando, RRazzano, MRea, NReimer, AReimer, OReposeur, TRitz, SRochester, LSBlandford, RDRodriguez, AYRomani, RWRoth, MRyde, FSadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMSgrò, CSmith, DABloom, EDSmith, PDSpandre, GSpinelli, PStarck, JLStrickman, MSSuson, DJTajima, HTakahashi, HTanaka, TThayer, JBBonamente, EThayer, JGThompson, DJTibaldo, LTorres, DFTosti, GTramacere, AUchiyama, YUsher, TLVasileiou, VVilchez, NBorgland, AWVitale, VWang, PWebb, NWiner, BLWood, KSYlinen, TZiegler, MBregeon, JBrez, ABrigida, MBruel, PBurnett, THCaliandro, GACameron, RACaraveo, PACasandjian, JMCecchi, CÇelik, ÖCharles, EChaty, SChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JConrad, JCutini, SDermer, CDDe Palma, FDigel, SWDormody, MDo Couto E Silva, EDrell, PSDubois, RDumora, DFarnier, CFavuzzi, CFegan, SJFocke, WBFrailis, MFukazawa, YFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiebels, BGiglietto, NGiordano, FGlanzman, TGodfrey, GGrenier, IAGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHayashida, MHays, EHoran, DHughes, REJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNKamae, TKatagiri, HKawai, NKerr, MKnödlseder, JKuehn, FKuss, MLande, JLatronico, LLemoineGoumard, MLongo, FLoparco, FLott, BLovellette, MNLubrano, PMakeev, AMazziotta, MNMcconville, WMcenery, JEMeurer, CMichelson, PFMitthumsiri, WMizuno, T
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. 845-848 How to Cite?
AbstractWe report the detection of gamma-ray emissions above 200 megaelectron volts at a significance level of 17s from the globular cluster 47 Tucanae, using data obtained with the Large Area Telescope onboard the Fermi Gamma-ray Space Telescope. Globular clusters are expected to emit gamma rays because of the large populations of millisecond pulsars that they contain. The spectral shape of 47 Tucanae is consistent with gamma-ray emission from a population of millisecond pulsars. The observed gamma-ray luminosity implies an upper limit of 60 millisecond pulsars present in 47 Tucanae.
Persistent Identifierhttp://hdl.handle.net/10722/188366
ISSN
2015 Impact Factor: 34.661
2015 SCImago Journal Rankings: 13.217
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAtwood, WBen_US
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dc.contributor.authorBaldini, Len_US
dc.contributor.authorBallet, Jen_US
dc.contributor.authorBarbiellini, Gen_US
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dc.contributor.authorBaughman, BMen_US
dc.contributor.authorBechtol, Ken_US
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dc.contributor.authorMorselli, Aen_US
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dc.contributor.authorMurgia, Sen_US
dc.contributor.authorNolan, PLen_US
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dc.contributor.authorNuss, Een_US
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dc.contributor.authorBellazzini, Ren_US
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dc.contributor.authorMcconville, Wen_US
dc.contributor.authorMcenery, JEen_US
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dc.contributor.authorMichelson, PFen_US
dc.contributor.authorMitthumsiri, Wen_US
dc.contributor.authorMizuno, Ten_US
dc.date.accessioned2013-09-03T04:03:57Z-
dc.date.available2013-09-03T04:03:57Z-
dc.date.issued2009en_US
dc.identifier.citationScience, 2009, v. 325 n. 5942, p. 845-848en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188366-
dc.description.abstractWe report the detection of gamma-ray emissions above 200 megaelectron volts at a significance level of 17s from the globular cluster 47 Tucanae, using data obtained with the Large Area Telescope onboard the Fermi Gamma-ray Space Telescope. Globular clusters are expected to emit gamma rays because of the large populations of millisecond pulsars that they contain. The spectral shape of 47 Tucanae is consistent with gamma-ray emission from a population of millisecond pulsars. The observed gamma-ray luminosity implies an upper limit of 60 millisecond pulsars present in 47 Tucanae.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.titleDetection of high-energy gamma-ray emission from the globular cluster 47 tucanae with Fermien_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.1177023en_US
dc.identifier.pmid19679807-
dc.identifier.scopuseid_2-s2.0-68949206508en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-68949206508&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume325en_US
dc.identifier.issue5942en_US
dc.identifier.spage845en_US
dc.identifier.epage848en_US
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