Fig. 5.
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LC II/LCO(1−0) ratio as a function of the metallicity (left) and specific SFR (right). IZw18 (red star) is compared to the galaxies compiled in Zanella et al. (2018, see references therein). The errorbar reflects the uncertainties of stellar mass and SFR. Pearson’s correlation coefficients for the regression fits are shown in each panel.
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