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Fig. B.1.

image

EW(Hα) maps for the 12 galaxies from our MaNGA sample containing HII blobs with auroral line detections (see Sect. 2). HII blobs are shown and numbered in each panel. White ellipses signify HII blobs with S/N[OIII]λ4363 ≥ 3.0, which are used for our Te analysis in Sect. 4.3.

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