Fig. 10
EW(Hα) vs. log([Nii]λ6584/Hα) for NGC 6762. The left and right panels show the spaxels with F(Hα)/F(Hα)peak ≤ 0.20 and 0.20 ≲ F(Hα)/F(Hα)peak ≲ 1.00, respectively. SF = pure star-forming galaxies; sAGN = strong AGN; wAGN = weak AGN; RG = retired galaxies. The dividing lines are transpositions of the SF/AGN borders from Kewley et al. (2001, 2006) and Stasińska et al. (2006), and the Kewley et al. (2006) Seyfert/LINER division (see Cid Fernandes et al. 2010).
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