Fig. 25.
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[Mg/Fe] − [Fe/H] distribution for A2A and APOGEE stars in intervals of vertical height (in kpc), for the inner bulge (left column), long bar-outer bulge region (middle column), and within a galactocentric radius of 3.5 kpc (right column). The stars in the first two columns are required to have |Ybar| < 1 kpc. For plot specifics, see the caption of Fig. 24.
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