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Fig. 15
Comparison of our integrated-light [Ca/Fe], [Ti/Fe], [Cr/Fe], and [Ba/Fe] abundance ratios with data for individual Milky Way stars (V2014, I2013: Venn et al. 2004; Ishigaki et al. 2013) and literature data for globular clusters (P2005, R2014: Pritzl et al. 2005; Roediger et al. 2014).
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