Fig. A.1.
2D distribution of the CH II fraction values of the pixels at the MUSE native resolution in NGC 1512 as defined in Eq. (2), as a function of the log Hα flux surface density of each pixel, in units of 10−20 erg s−1 cm−2 pc2. The black solid line shows the best-fitting parametrization, as described in Eq. (3). The obtained f0 and β parameters are shown in the top of the panel.
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