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Fig. 3.

image

Ratios of n-capture elements to Ba as a function of [Ba/H]. Symbols and Sculptor references are the same as in Fig. 1, but open squares are confirmed Milky Way CEMP stars with [Ba/Mg] >  0. The [Eu/Ba] ratio of the pure r-process is shown with a green dashed line, and the pure s-process is in orange (Bisterzo et al. 2014). In the case of [Y/Ba] the value of the r-rich star CS 22892-052 is also shown with a green dotted line (Sneden et al. 2003). Milky Way references: Reddy et al. (2003, 2006), Venn et al. (2004), François et al. (2007), Hansen et al. (2012), Mishenina et al. (2013), Roederer et al. (2014).

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