Fig. 14.
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[Mg/Fe] distributions predicted by the ES21 model computed at 8 kpc (green histogram) and by the M2 model of ES20 (magenta histogram) compared with the APOGEE DR16 data (black empty histogram) for stars with Galactocentric distances of between 6 and 10 kpc. Black, green, and magenta vertical dashed lines indicate the median values of the data and models.
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