Fig. 16.
[Eu/Ba] as an indicator of the s-process contribution to Ba. Red symbols indicate stars with unreasonable parallax. The gray band shows the highly r-process enriched star CS 22892−052 (Sneden et al. 2003). Gray dots indicate stars of the MW (Reddy et al. 2003, 2006; Cayrel et al. 2004). The median error is indicated in the lower left of each panel.
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