Fig. 3.
Evolution of different energy densities in the CF during a JCI. For tLF ≲ 2 × 105 s the synchrotron cooling is dominant (followed by SSC, not considered in the model). For tLF ≳ 2 × 105 s the BLR photon field dominates the cooling of electrons that interact in the Thomson regime. The grey shaded area represents the radiatively efficient stage in the OF.
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