Fig. 1.
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Results from a CLOUDY simulation (Ashwani Pandey; private commun.) showing the Hβ line emissivity as a function of the incident photon flux ϕ (computed from the 2.5D FRADO model) reaching a BLR cloud. The blue points represent simulation outputs, while the red curve shows a logarithmic fit, highlighting a clear nonlinear relationship.
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