Fig. 14.
Abundance distribution of light-s (X = Y, Zr) and heavy-s (X = Ba, La, Ce, Nd) elements for CEMP-s (blue) and CEMP-rs (red) stars. The box extends from the lower to upper [X/Fe] quartile, with a small horizontal line at the median. The whiskers extend from the box to show the full range of the data.
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