Fig. 13.
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Comparison of distributions of [Mg/Fe] (top panels) and [Si/Fe] (bottom panels) vs. [Fe/H] for our targeted MC substructure regions against those for large Milky Way satellites also using APOGEE data: the LMC, SMC, Sagittarius dSph, Fornax dSph, and the GSE. The left panels show individual stars for each substructure and the right panels show the mean and standard deviation for each substructure region. The overplotted lines show the chemical evolution track for each dwarf galaxy as determined by Hasselquist et al. (2021).
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