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Table 1.

Local thermodynamic equilibrium abundances of BPM 3066.

El Z ion A(X) Nlines A(X) [X/H] σ [X/Fe] NLTE Ref.
Li 3 0 3.28 2 3.00 0.09
Be 4 1 1.38 2 2.10 0.20
NH 7 0 7.86 band 6.10 −1.76 0.20 −0.19
OH 8 0 8.76 40 7.49 −1.27 0.31 0.30
Na 11 0 6.30 3 4.92 −1.38 0.16 0.19
Mg 12 0 7.54 2 6.59 −0.95 0.20 0.62 0.02 Bergemann et al. (2017)
Al 13 0 6.47 2 5.89 −0.58 0.02 0.99
Si 14 0 7.52 8 7.12 −0.40 0.03 1.17 −0.01 Bergemann et al. (2013)
Si 14 1 7.52 3 7.32 −0.20 0.07 1.32
Ca 20 0 6.33 19 5.15 −1.18 0.06 0.39 0.05 Mashonkina et al. (2007)
Sc 21 0 3.10 1 2.00 −1.10 0.20 0.47
Sc 21 1 3.10 8 2.09 −1.01 0.11 0.51
Ti 22 0 4.90 13 3.69 −1.21 0.07 0.36 0.31 Bergemann (2011)
Ti 22 1 4.90 28 3.73 −1.17 0.15 0.35 0.01 Bergemann (2011)
V 23 0 4.00 1 3.05 −0.95 0.20 0.62
V 23 1 4.00 6 2.67 −1.33 0.22 0.19
Cr 24 0 5.64 7 4.09 −1.55 0.12 0.02 0.27 Bergemann & Cescutti (2010)
Cr 24 1 5.64 8 4.33 −1.31 0.06 0.21
Mn 25 0 5.37 6 3.47 −1.90 0.17 −0.33
Mn 25 1 5.37 3 3.71 −1.66 0.01 −0.14
Fe 26 0 7.52 196 5.95 −1.57 0.12 0.04 Bergemann et al. (2012)
Fe 26 1 7.52 20 6.00 −1.52 0.11
Co 27 0 4.92 17 3.33 −1.59 0.15 −0.02 0.45 Bergemann et al. (2010)
Ni 28 0 6.23 21 4.79 −1.44 0.27 0.13
Ni 28 1 6.23 1 4.98 −1.25 0.20 0.27
Cu 29 0 4.21 3 2.64 −1.57 0.03 0.00
Zn 30 0 4.62 2 3.22 −1.40 0.07 0.17
Sr 38 1 2.92 2 2.05 −0.87 0.05 0.65
Y 39 1 2.21 7 1.38 −0.83 0.10 0.69
Zr 40 1 2.62 4 1.88 −0.74 0.09 0.78
Ba 56 1 2.17 1 1.70 −0.47 0.20 1.05

Notes. The adopted solar abundances are from Lodders et al. (2009), except for N, O, and Fe, which are from Caffau et al. (2011b), and Zn, which is from Caffau et al. (2011a). Li is from the Orgueil CI-chondrite (Lodders et al. 2009)

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