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Fig. 2.

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Abundances for the six stars analysed here (pink stars) compared to abundances for carbon-normal Carina stars (filled green circles), CEMP stars in Carina (yellow and cyan circles), carbon-normal MW halo stars (small grey circles), and CEMP MW halo stars (small black circles). All literature abundances have been converted to the Asplund et al. (2009) solar abundance scale, and all C abundances corrected for evolutionary effects following Placco et al. (2014).

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