Fig. 16.
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SSF-corrected symmetrised mean [Fe/H] (top row) and [Mg/Fe] (bottom row) distribution in the Xbar − Z plane for combined A2A and APOGEE stars with [Fe/H] > −1 dex in slices of |Ybar|. The dotted white lines trace the density distribution obtained from a Portail et al. (2017a) bulge-bar model. The red arrow points in the direction of the Sun.
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