Compton-induced HE – VHE γ-rays from pair cascade emissions in the SEDs of radio galaxies: NGC 1275
In the scheme of active galactic nuclei (AGNi), the blazar subclass is particularly bright in γ-rays. This is because of their emissions being beamed into our line of sight, as opposed to their misaligned parent population, radio galaxies. This work presents results of a Monte-Carlo code that propagates jet-collimate...