Fig. A.1
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Comparison between [X/Fe] vs [Fe/H] observed abundance patterns for light elements in the SMC. Orange dots are from Mucciarelli et al. (2023a), whereas grey diamonds are APOGEE DR17 data (Hasselquist et al. 2021). Orange and black contour lines represent density lines of the observed stellar distributions in Mucciarelli et al. (2023a) and Hasselquist et al. (2021), respectively.
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