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Fig. 11

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Violin plots for the star formation properties. Top: SFE. Centre: DGF. Bottom: Clump luminosity-to-mass ratio (Lclump/Mclump) distributions for different morphologies. The violin plots present the density of the data at different values, which is smoothed through the kernel density estimator. The upper, lower, and middle horizontal lines in the plots represent the highest, lowest, and median values, respectively.

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