Fig. 14.

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Radial profiles of the ΣM⋆, ΣSFR, and sSFR of the AGN and SF samples, sub-sampled on the basis of B/D. The higher the B/D ratio, the more dominant the bulge is in a galaxy. Both samples exhibit decreasing ΣM⋆ and ΣSFR profiles (top two rows). In DD and PB systems, AGN seem to demonstrate a increasing sSFR profile up to 1Re whereas the profiles are flat for both samples in BD galaxies (bottom row). Error bars represent the 3σ confidence intervals.
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