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. 2011 Nov 25;334(6059):1103-7.
doi: 10.1126/science.1210311.

A cocoon of freshly accelerated cosmic rays detected by Fermi in the Cygnus superbubble

M Ackermann  1 M AjelloA AllafortL BaldiniJ BalletG BarbielliniD BastieriA BelfioreR BellazziniB BerenjiR D BlandfordE D BloomE BonamenteA W BorglandE BottaciniM BrigidaP BruelR BuehlerS BusonG A CaliandroR A CameronP A CaraveoJ M CasandjianC CecchiA ChekhtmanC C CheungJ ChiangS CipriniR ClausJ Cohen-TanugiA de AngelisF de PalmaC D DermerE do Couto E SilvaP S DrellD DumoraC FavuzziS J FeganW B FockeP FortinY FukazawaP FuscoF GarganoS GermaniN GigliettoF GiordanoM GirolettiT GlanzmanG GodfreyI A GrenierL GuillemotS GuiriecD HadaschY HanabataA K HardingM HayashidaK HayashiE HaysG JóhannessonA S JohnsonT KamaeH KatagiriJ KataokaM KerrJ KnödlsederM KussJ LandeL LatronicoS-H LeeF LongoF LoparcoB LottM N LovelletteP LubranoP MartinM N MazziottaJ E McEneryJ MehaultP F MichelsonW MitthumsiriT MizunoC MonteM E MonzaniA MorselliI V MoskalenkoS MurgiaM Naumann-GodoP L NolanJ P NorrisE NussT OhsugiA OkumuraE OrlandoJ F OrmesM OzakiD PanequeD ParentM Pesce-RollinsM PierbattistaF PironM PohlD ProkhorovS RainòR RandoM RazzanoT ReposeurS RitzP M Saz ParkinsonC SgròE J SiskindP D SmithP SpinelliA W StrongH TakahashiT TanakaJ G ThayerJ B ThayerD J ThompsonL TibaldoD F TorresG TostiA TramacereE TrojaY UchiyamaJ VandenbrouckeV VasileiouG VianelloV VitaleA P WaiteP WangB L WinerK S WoodZ YangS ZimmerS Bontemps
Affiliations

A cocoon of freshly accelerated cosmic rays detected by Fermi in the Cygnus superbubble

M Ackermann et al. Science. .

Abstract

The origin of Galactic cosmic rays is a century-long puzzle. Indirect evidence points to their acceleration by supernova shockwaves, but we know little of their escape from the shock and their evolution through the turbulent medium surrounding massive stars. Gamma rays can probe their spreading through the ambient gas and radiation fields. The Fermi Large Area Telescope (LAT) has observed the star-forming region of Cygnus X. The 1- to 100-gigaelectronvolt images reveal a 50-parsec-wide cocoon of freshly accelerated cosmic rays that flood the cavities carved by the stellar winds and ionization fronts from young stellar clusters. It provides an example to study the youth of cosmic rays in a superbubble environment before they merge into the older Galactic population.

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Comment in

  • Astronomy. Cosmic-ray origins.
    Binns WR. Binns WR. Science. 2011 Nov 25;334(6059):1071-2. doi: 10.1126/science.1213490. Science. 2011. PMID: 22116872 No abstract available.

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