An impulsive-injection diffusion-loss model fitted to Vela X data gives a diffusion coefficient of 1e26 cm2/s at 10 TeV, more than 1000 times slower than in the ISM.
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Most cataloged Fermi point sources in the Vela region are spurious; the GeV emission is extended hadronic emission from the supernova remnant.
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On the Gamma-Ray Nebula of Vela Pulsar. I. Very Slow Diffusion of Energetic Electrons within the TeV Nebula
An impulsive-injection diffusion-loss model fitted to Vela X data gives a diffusion coefficient of 1e26 cm2/s at 10 TeV, more than 1000 times slower than in the ISM.
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GeV emission in the region of Vela: a new view of the supernova remnant
Most cataloged Fermi point sources in the Vela region are spurious; the GeV emission is extended hadronic emission from the supernova remnant.