Fig. 5

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Photospheric abundances for EC 22536–5304 A relative to solar values from Asplund et al. (2009). Abundance measurements are shown as black dots, while upper limits are marked with grey arrows. Solid red lines show the corresponding metal abundances adopted in our model for EC 22536–5304 B, as given by the best-fit [Fe/H] and [α∕Fe ]. The solar reference is indicated by the dashed grey line.
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