Fig. 16.
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[El/Eu] vs. [Fe/H] for the mixed elements: Mo, Pr, and Nd. Data for both the field-star sample and OC sample are shown. The symbols and colours are the same as in Fig. 4. The dashed yellow lines track the pure contribution of the r-process derived using the solar abundances from Grevesse et al. (2007), and the most recent percentages from Prantzos et al. (2020) for the r-process and the r- + p-process for Mo.
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