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Fig. 7


AGN properties for each spectral type and reported accretion rates. As can be seen, strongly (solid line) and weakly (dashed) accreting LINERs show a larger difference in underdensities. Transition objects with high accretion rate have more powerful starburst and smaller concentration indices at high densities (irregular galaxies). Seyferts show a transition at ln (1 + δ) ≈−0.7.

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