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Fig. 6

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Mean heavy element (Z> 38) distribution of the NGC 5897 stars. The different lines are the solar-scaled (S.S.) abundances from Simmerer et al. (2004), normalized to Ba. We also indicate the best fit to our measurements that is obtained by admixing 13% of s-process material. The red open circles show the abundances for star S-138, which is low in Eu.

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