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Fig. 7

image

Run of the [C/Fe] and [N/Fe] abundance ratio versus extinction-corrected visual magnitude in four bins of metallicity for Sculptor stars, with the black asterisks denoting objects belonging to the kinematic substructure. The vertical line indicates the location of the RGB bump (where deep mixing onsets) for the metal-poor and metal-rich component of Sculptor (see Majewski et al. 1999).

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