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. 2009 Aug 14;325(5942):845-8.
doi: 10.1126/science.1177023.

Detection of high-energy gamma-ray emission from the globular cluster 47 Tucanae with Fermi

A A Abdo  1 M AckermannM AjelloW B AtwoodM AxelssonL BaldiniJ BalletG BarbielliniD BastieriB M BaughmanK BechtolR BellazziniB BerenjiR D BlandfordE D BloomE BonamenteA W BorglandJ BregeonA BrezM BrigidaP BruelT H BurnettG A CaliandroR A CameronP A CaraveoJ M CasandjianC CecchiO CelikE CharlesS ChatyA ChekhtmanC C CheungJ ChiangS CipriniR ClausJ Cohen-TanugiJ ConradS CutiniC D DermerF de PalmaS W DigelM DormodyE do Couto e SilvaP S DrellR DuboisD DumoraC FarnierC FavuzziS J FeganW B FockeM FrailisY FukazawaP FuscoF GarganoD GasparriniN GehrelsS GermaniB GiebelsN GigliettoF GiordanoT GlanzmanG GodfreyI A GrenierJ E GroveL GuillemotS GuiriecY HanabataA K HardingM HayashidaE HaysD HoranR E HughesG JóhannessonA S JohnsonR P JohnsonT J JohnsonW N JohnsonT KamaeH KatagiriN KawaiM KerrJ KnödlsederF KuehnM KussJ LandeL LatronicoM Lemoine-GoumardF LongoF LoparcoB LottM N LovelletteP LubranoA MakeevM N MazziottaW McConvilleJ E McEneryC MeurerP F MichelsonW MitthumsiriT MizunoA A MoiseevC MonteM E MonzaniA MorselliI V MoskalenkoS MurgiaP L NolanJ P NorrisE NussT OhsugiN OmodeiE OrlandoJ F OrmesD PanequeJ H PanettaD ParentV PelassaM PepeM PierbattistaF PironT A PorterS RainòR RandoM RazzanoN ReaA ReimerO ReimerT ReposeurS RitzL S RochesterA Y RodriguezR W RomaniM RothF RydeH F-W SadrozinskiD SanchezA SanderP M Saz ParkinsonC SgròD A SmithP D SmithG SpandreP SpinelliJ-L StarckM S StrickmanD J SusonH TajimaH TakahashiT TanakaJ B ThayerJ G ThayerD J ThompsonL TibaldoD F TorresG TostiA TramacereY UchiyamaT L UsherV VasileiouN VilchezV VitaleP WangN WebbB L WinerK S WoodT YlinenM Ziegler
Affiliations

Detection of high-energy gamma-ray emission from the globular cluster 47 Tucanae with Fermi

A A Abdo et al. Science. .

Abstract

We report the detection of gamma-ray emissions above 200 megaelectron volts at a significance level of 17sigma 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.

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