Fig. 9.
Hertzsprung-Russell diagram for all CEMP-no and CEMP-s stars, with the same symbols and colour-coding as in Fig. 8. Because the narrow giant branch is very crowded, we additionally show for the CEMP-no stars the stacked histogram for logg on the side, where dark grey are binary and light grey are single stars. Typical error bars are indicated in the top left corner.
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