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Fig. 10


Correlations between Al–Mg (left and middle panels) and between Na–O (right panel). Cepheid stars (filled circles) are compared with field dwarfs from the thin disk analyzed by Reddy et al. (2003, R03, magenta squares), from the thin (dark green diamonds) and thick (light green diamonds) disks analyzed by Bensby et al. (2005, B05), and from the thin (black crosses) and thick (orange pluses) disks analyzed by Mikolaitis et al. (2014, M14).

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