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Fig. A.1.

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Metallicity gradients, 12+log(O/H) and log(N/O), in our sample of LINER-like galaxies. 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. Red vertical lines mark the break point, and red shaded areas their corresponding uncertainty.

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