Fermi gamma-ray "bubbles" from stochastic acceleration of electrons.
Gamma-ray data from Fermi Large Area Telescope reveal a bilobular structure extending up to ∼50° above and below the Galactic Center. It has been argued that the gamma rays arise from hadronic interactions of high-energy cosmic rays which are advected out by a strong wind, or from inverse-Compton sc...
| Main Authors: | , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2011
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