Fig. 1.

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Diagnostic diagrams of the central spaxels in our sample of galaxies. The color bar shows the equivalent width for Hα (WHα). The solid and dashed lines represent the region limits as defined by Kewley et al. (2006), with the exception of the separation between Seyfert 2 and LINERs in the [NII]/Hα diagram, which was taken from Cid Fernandes et al. (2010). Each region is labeled as follows: SFG for star-forming galaxies, SEY for Seyferts, LIN for LINERs, and COM for composites.
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