Fig. 5
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LTE barium abundance as function of υmic for the subordinate lines 5853, 6141, and 6496 Å. Each trend is related to one star and is colour-coded according to log g. Shades enclose the most probable ranges of A(Ba) of the TO-1 and TO-2 stars; see main text. Dashed gray and red lines indicate the mean A(Ba) in the shades for each star, respectively.
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