Table 1
Chemical composition of BD+46°442.
Z | Ion | log ϵ | [X/H] | rms | Δ[X/H] | N | Flag | |
|
||||||||
A | B | |||||||
|
||||||||
6 | C I | 8.11 | −0.41 | 0.09 | −0.05 | + 0.05 | 6 | 2 |
7 | N I | 7.89 | −0.04 | 0.18 | + 0.02 | −0.01 | 2 | 3 |
11 | Na I | 5.79 | −0.53 | 0.08 | −0.09 | + 0.09 | 2 | 3 |
12 | Mg I | 6.92 | −0.66 | 0.35 | −0.07 | + 0.07 | 2 | 3 |
13 | Al I | 6.32 | −0.15 | − | −0.09 | + 0.09 | 1 | 3 |
14 | Si I | 7.09 | −0.45 | 0.16 | −0.08 | + 0.07 | 8 | 2 |
16 | S I | 6.67 | −0.45 | 0.08 | −0.06 | + 0.06 | 3 | 2 |
20 | Ca I | 5.51 | −0.85 | 0.08 | −0.11 | + 0.12 | 5 | 2 |
21 | Sc II | 2.38 | −0.77 | 0.15 | −0.25 | + 0.26 | 4 | 1 |
22 | Ti I | 4.40 | −0.61 | − | −0.17 | + 0.16 | 1 | 3 |
22 | Ti II | 4.27 | −0.74 | 0.17 | −0.25 | + 0.24 | 13 | 1 |
23 | V II | 3.30 | −0.67 | 0.16 | −0.23 | +0.23 | 3 | 1 |
24 | Cr I | 4.75 | −0.86 | 0.13 | −0.17 | + 0.16 | 3 | 2 |
24 | Cr II | 4.86 | −0.73 | 0.10 | −0.17 | +0.18 | 9 | 1 |
25 | Mn I | 4.52 | −0.86 | 0.12 | −0.14 | +0.14 | 3 | 2 |
26 | Fe I | 6.59 | −0.88 | 0.20 | −0.13 | +0.13 | 39 | 2 |
26 | Fe II | 6.75 | −0.73 | 0.15 | −0.18 | +0.19 | 25 | 1 |
28 | Ni I | 5.37 | −0.86 | 0.13 | −0.14 | + 0.13 | 15 | 2 |
29 | Cu I | 2.89 | −1.32 | − | −0.20 | + 0.21 | 1 | 3 |
30 | Zn I | 3.72 | −0.85 | − | −0.16 | + 0.18 | 1 | 3 |
39 | Y II | 1.03 | −1.19 | 0.12 | −0.27 | + 0.27 | 3 | 1 |
40 | Zr II | 1.79 | −0.79 | − | −0.25 | + 0.25 | 1 | 3 |
56 | Ba II | 1.40 | −0.73 | − | −0.31 | + 0.30 | 1 | 3 |
60 | Nd II | 1.07 | −0.49 | − | −0.28 | + 0.29 | 1 | 3 |
63 | Eu II | 0.02 | −0.48 | − | −0.26 | + 0.27 | 1 | 3 |
Notes. Abundances are given for our best-fit photospheric model Teff/log g/Vtur = 6250/1.5/4.0. Δ[X/H] designates abundance changes corresponding to the changes in Teff/log g of −250 K/−0.5 dex (case A) and + 250 K/+0.5 dex (case B), which are our second best atmospheric model estimates. The flag designates the quality of the N lines used in the averaging, from one for the best cases to three for the worst. Elements with flag 3 had fewer than three lines with EW ≤ 50 mÅ.
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