Image Details
Caption: Figure 1.
Electron cooling time in the galaxy frame as a function of γ. Top panel: blazar emission site located in the BLR. Bottom panel:
blazar located in the MT. Broken lines represent the various cooling mechanisms and the solid black line is the total cooling
time. Plots were calculated for seed photon energies
0, BLR = 3 × 10
−5 and
0, MT = 5 × 10
−7, seed photon energy densities
U
BLR = 10
−2 erg cm
−3,
U
MT = 10
−4 erg cm
−3, and magnetic field energy
U
B
= 100
U
EC.
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