Simulating the transport of relativistic electrons and magnetic fields injected by radio galaxies in the intracluster medium

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Fig. 14.

Evolution of the spectral energy distributions of electrons emitted by the radio galaxy in Run1, for three different acceleration and cooling models (colours) and for three different radial ranges: r ≤ 300 kpc (solid), 300 kpc < r ≤ 600 kpc (dashed), and r > 600 kpc (dotted).

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