Uncertainties on derived [Mn/Fe] for the metal-poor star B3-b1 and the red clump star BWc-6.
|Star||T eff||log g||[Fe/H]||v t||Ref.||[Mn1/Fe]||[Mn2/Fe]||[Mn3/Fe]||[Mn4/Fe]||[Mn/Fe]|
Reference. (1) Lecureur et al. (2007) (present results); (2) Zoccali et al. (2008); (3) Ryde et al. (2010); (4) Hill et al. (2011) GIRAFFE data; (5) Hill et al. (2011) UVES data (present results). [Mn/Fe] is also derived with changes in model parameters of ΔTeff = −150 K, Δlog g = 0.2, Δvt = 0.1 km s-1, Δ[Fe/H] = −0.1 dex. We note that star B3-b1 was chosen for its reanalysis by Ryde et al. (2010), but it has one discardable line that gives a low Mn (in parenthesis) to which a low weight is given since it disagrees with the other three lines, and only an extra − 0.05 dex is added to the mean of the other three lines.
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