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Fig. 7.


Fraction of R > −0.6 as a function of stellar mass, (MuMr) color, Dn(4000) parameter, or log(MBH) (a, b, c, and d, respectively), for barred AGN galaxies (solid lines), AGNs in pair systems (dashed lines), and unbarred AGNs in the control sample (dotted lines). Each bin for each sample contains a similar number of galaxies. The average number of galaxies in each bin is ≈93 for barred-agn, ≈270 for agn in pairs and ≈110 for CS.

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