Fig. 8.
Spatial location of the Hα bright regions that show inconsistency with models of star forming galaxies (in black; star symbols in Fig. 7) or having a ratio [OIII]5007/Hα > 0.5 or [SII]6731/Hα > 0.4 (orchid and green respectively; filled stars in Fig. 7) overlaid on an RGB image of the gas emission (R: Hα, G: [SII]6716,6731, B: [OIII]4959,5007).
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