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Fig. 10

image

Distributions of log (Lum [OIII] /L) for barred AGN (solid lines) and unbarred active galaxies (full surfaces) with different host group color ranges: (MuMr)Groups> 2.4 and (MuMr)Groups< 2.4 (upper and middle panels, respectively). Lower panel shows mean log (Lum(OIII) /L) as a function of the host group colors for AGN galaxies with and without bars in groups (solid and dashed lines, respectively).

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