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

Open Access

Fig. 5

NLTE (stars) and LTE (open circles) abundance ratios [Pd/Fe] for the sample stars. The smaller and larger symbols correspond to the dwarfs (log g > 3.0) and the giants (log g ≤ 3.0), respectively. For each star, the error bar corresponds to σ_tot.

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