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Fig. 6

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[O/Fe] and [Mg/Fe] vs. [Fe/H] diagrams for various LMC populations: abundances measured in SNRs (ISM gas phase, this work) are shown with red pentagons. The crosses indicate median error bars. Blue open circles are the old globular clusters from Johnson et al. (2006, ages ~. Chemical abundances of Bar and disc stars are marked by black squares and grey dots, respectively (from Van der Swaelmen et al. 2013, ages 1 Gyr).

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