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Fig. 6


Chemical element patterns for ALW-8 (red symbols) are shown for the lighter elements (top panel) and the neutron-capture element abundances (bottom panel). For comparison, we overplotted the CEMP-no star in the Sculptor dSph (Skúladóttir et al. 2015, blue diamonds), and the weak and main r-process stars HD 122563 (Honda et al. 2006, gray shades) and CS 22892-052 (Sneden et al. 2003, black dots). Here, all stars were placed on the same Solar scale. All ratios for the heavier elements were normalized to Y.

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