Fig. 8.

Relations between the radius and other parameters of the circumnuclear region of the AGN-type. Panels a, b, and e: radius of the zone of dominant contribution of the AGN to the radiation, RAGN, as a function of the luminosity of this zone in the Hα emission line (panel a), in the [O III]λλ4959,5007 emission lines (panel b), and as a function of the central gas velocity dispersion (panel e). Panel c, d, and f: same as panels a, b, e (respectively) but for the radius of the zone of the AGN influence on the radiation, RINT. The points in each panel denote individual galaxies. The line is the best linear fit to those data (see Table 3).
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