Fig. 20.
Abundances [Pb/hs] and [ls/hs] as a function of [Mg/hs], where [ls] = 1/2([Y/Fe]+[Zr/Fe]) and [hs/Fe] = 1/2([La/Fe]+[Ce/Fe]). The measured abundances are colour-coded as in Fig. 7, empty squares as in Fig. 15, and the model predictions as in Fig. 13. Blue and red triangles represent CEMP-s and CEMP-rs stars from the literature.
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