Fig. 2
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Comparison around the 4810.5 Å Zn (left panel) and the 6645.1 Å EuII (right panel) lines between the observed spectra and seven synthetic spectra computed assuming the derived atmospheric parameters for each star and varying the level of [Zn/Fe] and [EuII/Fe]. The variations are computed with respect to the abundances measured in Rup106.
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