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Fig. B.1.

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Diagram of log(N/O) vs. 12+log(O/H) for the HII regions in our sample of LINERs. The colorbar shows the distance to the galactic center in terms of R50. Nuclear estimations of the corresponding chemical abundance ratio are represented as follows: green triangles are the estimations from AGN models with αOX = −1.6; orange and red stars are the estimations from pAGB models with Teff = 105 K and Teff = 1.5 ⋅ 105 K respectively; and black squares are the estimations from ADAF models. The solid back line represents the fit provided by Coziol et al. (1999), the dotted line shows the fit by Andrews & Martini (2013), and the dash-dotted line shows the fit by (Belfiore et al. 2015).

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