A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies

Open Access

Fig. 9.

Spatial distribution of the particles responsible for the peaks in SED. Top panel: position of the particle population with γ_max ∼ 10⁴ for case (a) (left), case (b) (middle), and case (c) (right). Bottom panel: position of the particle population with γ_max ∼ 10⁵ for case (a) (left), case (b) (middle), and case (c) (right).

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