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Fig. 9.
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[Mg/Fe] abundance ratios as a function of [Fe/H] for substructure C (GE) from APOGEE DR16. We use different symbols for the different clusters. Colours for the groups (C1 to C5) follow Fig. 8. The small dots show abundances of all the halo stars within 2.5 kpc in APOGEE DR16.
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