Extended gamma-ray emission from particle escape in pulsar wind nebulae - Application to HESS J1809–193 and HESS J1825–137

Open Access

Fig. 4.

Evolution of the spatial diffusion coefficient at 100 TeV in the different model setups. For reference, the effective value of the diffusion coefficient at 100 TeV for large-scale transport in the Galactic disk is on the order of 10³⁰ cm² s⁻¹.

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