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Fig. 6.

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W80 velocity vs L[OIII] for the MaNGA sample of 13 dwarf galaxies with AGN outflow candidates (red squares for AGN galaxies, red diamonds for SF-AGN galaxies), the AGN dwarf galaxy sample of Liu et al. (2020) (red triangles), the z < 2 type-2 AGN quasars of Harrison et al. (2014) (grey pluses), the radio-quiet quasars of Liu et al. (2013) (grey crosses), the z ∼ 2 type-1 massive AGN of Kakkad et al. (2020) (grey diamonds), the massive LLAGN of Heckler et al. (2022) (grey circle) and the MaNGA sample of low-intermediate luminosity massive galaxies of Wylezalek et al. (2020) (grey squares). The solid lines are regression fits to the massive sample (grey), the dwarf sample of AGN outflows, which includes the nine MaNGA dwarf galaxies with AGN outflows and those from Liu et al. (2020) (red), and the combination of all the massive galaxies, along with the dwarf sample of AGN outflows (purple) indicated as the shaded area the 1σ error of the regression line.

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