Fig. 2.

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Cooling and escape times for primary electrons (upper panels) and protons (bottom panels) as a function of energy in scenario (0). Left panels: typical case of a low SFR galaxy (Ṁ∗ = 0.1 M⊙ yr−1). Right panels: typical case of a high SFR system (Ṁ∗ = 10 M⊙ yr−1). Solid lines represent different cooling processes: synchrotron (pink), ionisation (yellow), Bremsstrahlung (red), IC (green), and p − p (blue). The black dashed lines are for diffusion, whereas the grey double-dot-dashed lines are for advection.
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