Fig. 22.
Distribution of the gas-phase oxygen abundances used for ESO 467-G051 H II regions, based on the D16, O3N2 and N2 calibrations. The dashed lines represent the median for each distribution and the black vertical line indicates the average abundance for Type II SNe hosts from the PISCO compilation using the D16 calibration (Galbany et al. 2018).
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