Fig. 13
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Flaring plots highlighting the behaviour of global and beam SFE (blue) and fmol (yellow). The symbols and conventions follow Fig. 7. While the evolution of the galaxies from the SF to the MX group is mostly driven by decrements of fmol, the significant drop (from MX to the nR/fR groups) in SFR in the centre of the galaxies is dominated by decrements of SFE.
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