Open Access
Fig. 16
Model NIR luminosities as a function of the MIR luminosity for the 1∕z winds with anisotropic illumination for a 
(left panel) and 2 (right panel) times smaller inner radius of the thin gas disk. The solid and dashed lines are the relations found by Burtscher et al. (2015) for type 1 and type 2 objects, respectively.
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