Fig. 11
Eu-normalized log ϵ(X) as a function of atomic number for the five IOCs. The solar element r-process and s-process abundance distributions from Simmerer et al. (2004) are shown as red and blue solid lines, respectively. The element names are listed in the bottom of the panel, and the error bars indicate the standard deviations of the seven s-process elements discussed in this work.
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