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Fig. 9

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Synthetic spectra for the Eu 4129 and 4205 Å lines for  [ Eu / H ]  =  − 2.80 and for the abundances calculated in three other studies of this star (see text). It is clear that they over estimate the strength of both lines. While the 4205 Å line includes several blends particularly V ii 4205.09 Å, the 4129 Å has none. We show the V ii line separately in the right-hand panel (dot-line).

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