Fig. 13
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Relation between the αCO vs. the gas-phase metallicity (left panel) and the clumpiness parameter (right panel), defined by Eq. (11). The Spearman correlation coefficients are calculated for the means of individual galaxies, shown by colored dots. We show the Galactic αCO value from B13 and the range of values compatible with it within 30% (gray-shaded area).
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