Understanding the origin of palladium in metal-poor stars based on the non-local thermodynamic equilibrium analysis of Pd I lines

Open Access

Fig. 8

Same as in Fig. 7 for the abundance ratios of Eu, Ba, Sr, and Pd. The long-dashed red and dash-dotted blue lines indicate the elemental ratios predicted by Prantzos et al. (2020) for pure r- and s-process, respectively. The short-dashed red line corresponds to the empirical r-process ratio [Sr/Ba]_r-II = −0.38.

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