Element, stellar abundances and line-to-line dispersion, and number of lines.
|Element, X||[X/Fe]||σ||No. lines|
|O I||−0.23||± 0.10||3|
|Na I||< 0 .85||–||2|
|Mg I||0.28||± 0.11||4|
|Ca I||0.26||± 0.10||6|
|Ti II||< 0.17||–||4|
|Cr I||−0.20 wa||± 0.10||2.5|
|Ba II||0.20||± 0.00||2|
Notes. A wa indicates that a weighted average is listed, where one of the three Cr lines is given a weight of 0.5.
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