Volume 562, February 2014
|Number of page(s)||14|
|Published online||13 February 2014|
Lines used in the abundance analysis.
Resulting abundances for the programme stars.
Abundance differences as a result of a Teff shift of +50 K, a log g shift of +0.05, a ξt shift of +0.2 km s-1 and effects on individual abundances due to line scatter.
© ESO, 2014
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