Fig. 12
Top panel: mean abundance pattern for NGC 6426. The color coding is the same as in Fig. 5. The red line and red shaded region state the abundances and uncertainties of HD 108317 as derived by Roederer et al. (2012). Both patterns are unscaled, i.e., represent their original values. Bottom panel: residual pattern for the cluster stars after subtracting HD 108317.
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