Looking for imprints of the first stellar generations in metal-poor bulge field stars

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Fig. 11

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[Y/Fe] (upper panel) and [Ba/Fe] (lower panel) abundance ratios as a function of the metallicity for the five sample stars, compared with literature abundances. Symbols are the same as in Fig. 8, in addition to the abundances from Van der Swaelmen et al. (2016; filled grey circles).

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