Fig. 16.
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Ratios of strong emission lines observed with MUSE. Top and centre: map of [O III] λ4959,5007/Hα obtained from a double component Gaussian fit to the emission lines. Bottom panel: map of [O I] λ6300/Hα obtained from a single Gaussian component fit. All maps have been corrected for extinction. The labelled features are discussed in Sect. 6.3. Maps of the full FoV are shown in Fig. B.2.
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