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Fig. 6
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Abundance corrections to A(C) derived from the EW of the CH G band between 4 297 and 4 303 Å. Panel A: final abundance correction ΔA(C) = A(C)3D CEMP − A(C)1D from 1D HE MARCS to 3D CEMP models. Panel B: A(C)3D CEMP − A(C)3D scaled-solar. Panel C: A(C)3D scaled-solar − A(C)1D.
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