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Fig. 3.


Panel a: [O III] and panel b: Hα emission of the total fitted line profile. Both maps have been obtained from the fit of the star-subtracted smoothed (with 1-spaxel σ Gaussian kernel) data cube; a signal-to-noise cut of 3 has been applied. The FOV covers ∼5.3 × 5.3 kpc2. The reported flux is per spaxel.

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