Hadronic emission from the environment of the Crab Pulsar Wind Nebula by re-accelerated particles

Open Access

Fig. 4.

Spectrum of re-accelerated protons that have escaped the PWN at the final time step. The Poisson errors on these measurements are shown. The x-axis errors denote the size of the bins. A power-law fit of E²dN/dE up to 1 PeV, normalised to 1 TeV, is shown for comparison to highlight the spectral break.

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