Fig. 8.
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Spatially resolved properties of the narrow component. From left to right: gas-phase metallicity (12 + log(O/H)), dust extinction (AV), and dust-corrected star formation rate surface density (ΣSFR) maps. The plus signs show the location of the three components identified in Figs. 4 and 5. The gray contours represent the 5, 25, and 75σ of the narrow [O III] flux from Fig. 6.
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