Table 2
Fe i and Fe ii abundances and standard deviations.
| Star | [FeI/H] | [FeII/H] |
|
|
||
| HD 4747 | −0.28 ± 0.06 | −0.28 ± 0.10 |
| HD 52756 | 0.09 ± 0.10 | 0.03 ± 0.15 |
| HD 74014 | 0.23 ± 0.07 | 0.16 ± 0.11 |
| HD 89707 | −0.35 ± 0.09 | −0.40 ± 0.12 |
| HD 167665 | −0.11 ± 0.10 | −0.09 ± 0.10 |
| HD 189310 | −0.03 ± 0.10 | −0.10 ± 0.22 |
| HD 211847 | −0.10 ± 0.06 | −0.11 ± 0.09 |
|
|
||
| HD 3277 | −0.10 ± 0.05 | −0.12 ± 0.08 |
| HD 17289 | −0.13 ± 0.08 | −0.09 ± 0.13 |
| HD 30501 | −0.09 ± 0.10 | −0.14 ± 0.18 |
| HD 43848 | 0.18 ± 0.13 | 0.14 ± 0.25 |
| HD 53680* | −0.37 ± 0.24 | −0.61 ± 0.41 |
| HD 154697 | 0.10 ± 0.06 | 0.06 ± 0.10 |
| HD 164427A | 0.15 ± 0.06 | 0.14 ± 0.09 |
| HIP 103019* | −0.34 ± 0.29 | −0.68 ± 0.45 |
|
|
||
| HD 74842 | −0.12 ± 0.09 | −0.10 ± 0.11 |
| HD 94340 | 0.10 ± 0.06 | 0.08 ± 0.11 |
| HD 112863 | −0.12 ± 0.09 | −0.14 ± 0.10 |
| HD 206505 | 0.10 ± 0.09 | 0.08 ± 0.12 |
Notes.
These stars were discarded from the abundance analysis because of the large scatter on the Fe i and Fe ii abundances which may be related to the fact that these stars are probably not well classified and may actually have lower Teff (see Sect. 5).
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