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. 2008 Nov 21;322(5905):1218-21.
doi: 10.1126/science.1165572. Epub 2008 Oct 16.

The Fermi Gamma-Ray Space Telescope discovers the pulsar in the young galactic supernova remnant CTA 1

A A Abdo  1 M AckermannW B AtwoodL BaldiniJ BalletG BarbielliniM G BaringD BastieriB M BaughmanK BechtolR BellazziniB BerenjiR D BlandfordE D BloomG BogaertE BonamenteA W BorglandJ BregeonA BrezM BrigidaP BruelT H BurnettG A CaliandroR A CameronP A CaraveoP CarlsonJ M CasandjianC CecchiE CharlesA ChekhtmanC C CheungJ ChiangS CipriniR ClausJ Cohen-TanugiL R CominskyJ ConradS CutiniD S DavisC D DermerA de AngelisF de PalmaS W DigelM DormodyE do Couto E SilvaP S DrellR DuboisD DumoraY EdmondsC FarnierW B FockeY FukazawaS FunkP FuscoF GarganoD GasparriniN GehrelsS GermaniB GiebelsN GigliettoF GiordanoT GlanzmanG GodfreyI A GrenierM-H GrondinJ E GroveL GuillemotS GuiriecA K HardingR C HartmanE HaysR E HughesG JóhannessonA S JohnsonR P JohnsonT J JohnsonW N JohnsonT KamaeY KanaiG KanbachH KatagiriN KawaiM KerrT KishishitaB KiziltanJ KnödlsederM L KocianN KominF KuehnM KussL LatronicoM Lemoine-GoumardF LongoV LonjouF LoparcoB LottM N LovelletteP LubranoA MakeevM MarelliM N MazziottaJ E McEneryS McGlynnC MeurerP F MichelsonT MineoW MitthumsiriT MizunoA A MoiseevC MonteM E MonzaniA MorselliI V MoskalenkoS MurgiaT NakamoriP L NolanE NussM OhnoT OhsugiA OkumuraN OmodeiE OrlandoJ F OrmesM OzakiD PanequeJ H PanettaD ParentV PelassaM PepeM Pesce-RollinsG PianoL PieriF PironT A PorterS RainòR RandoP S RayM RazzanoA ReimerO ReimerT ReposeurS RitzL S RochesterA Y RodriguezR W RomaniM RothF RydeH F-W SadrozinskiD SanchezA SanderP M Saz ParkinsonT L SchalkA SellerholmC SgròE J SiskindD A SmithP D SmithG SpandreP SpinelliJ-L StarckM S StrickmanD J SusonH TajimaH TakahashiT TakahashiT TanakaJ B ThayerJ G ThayerD J ThompsonS E ThorsettL TibaldoD F TorresG TostiA TramacereT L UsherA Van EttenN VilchezV VitaleP WangK WattersB L WinerK S WoodH YasudaT YlinenM Ziegler
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Free article

The Fermi Gamma-Ray Space Telescope discovers the pulsar in the young galactic supernova remnant CTA 1

A A Abdo et al. Science. .
Free article

Abstract

Energetic young pulsars and expanding blast waves [supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma-ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 x 10(-13) seconds per second. Its characteristic age of 10(4) years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma-ray sources associated with star-forming regions and SNRs are such young pulsars.

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