Table 3
Final metallicity of GBSs obtained via combination of individual line abundances of neutral lines corrected by NLTE effects.
| Star | [Fe/H] | σ Fe i | Δ (Teff) | Δ (log g) | Δ (vmic) | Δ (LTE) | Δ (ion) | σ Fe ii | N Fe i | N Fe ii |
|
|
||||||||||
| Metal-Poor | ||||||||||
| HD 122563 | –2.64 | 0.01 | 0.02 | 0.00 | 0.01 | +0.10 | –0.19 | 0.03 | 60 | 4 |
| HD 140283 | –2.36 | 0.02 | 0.04 | 0.02 | 0.00 | +0.07 | +0.04 | 0.04 | 23 | 2 |
| HD 84937 | –2.03 | 0.02 | 0.04 | 0.02 | 0.01 | +0.06 | –0.01 | – | 20 | 1 |
|
|
||||||||||
| FG dwarfs | ||||||||||
| δ Eri | +0.06 | 0.01 | 0.00 | 0.00 | 0.01 | +0.00 | +0.04 | 0.02 | 156 | 11 |
| ϵ For | –0.60 | 0.01 | 0.01 | 0.00 | 0.00 | +0.02 | +0.09 | 0.02 | 148 | 8 |
| α Cen B | +0.22 | 0.01 | 0.01 | 0.00 | 0.02 | +0.00 | +0.09 | 0.02 | 147 | 9 |
| μ Cas | –0.81 | 0.01 | 0.01 | 0.01 | 0.01 | +0.01 | +0.01 | 0.02 | 145 | 7 |
| τ Cet | –0.49 | 0.01 | 0.00 | 0.00 | 0.00 | +0.01 | +0.01 | 0.02 | 148 | 10 |
| 18 Sco | +0.03 | 0.01 | 0.01 | 0.00 | 0.01 | +0.02 | +0.00 | 0.02 | 158 | 10 |
| Sun | +0.03 | 0.01 | 0.00 | 0.00 | 0.00 | +0.01 | +0.04 | 0.02 | 150 | 9 |
| HD 22879 | –0.86 | 0.01 | 0.03 | 0.01 | 0.01 | +0.02 | –0.02 | 0.02 | 117 | 10 |
| α Cen A | +0.26 | 0.01 | 0.01 | 0.00 | 0.00 | +0.02 | +0.07 | 0.02 | 150 | 12 |
| μ Ara | +0.35 | 0.01 | 0.00 | 0.00 | 0.00 | +0.02 | +0.13 | 0.02 | 143 | 13 |
| β Hyi | –0.04 | 0.01 | 0.01 | 0.00 | 0.00 | +0.03 | +0.05 | 0.01 | 143 | 12 |
| β Vir | +0.24 | 0.01 | 0.01 | 0.00 | 0.01 | +0.03 | +0.06 | 0.02 | 148 | 10 |
| η Boo | +0.32 | 0.01 | 0.00 | 0.00 | 0.01 | +0.02 | +0.07 | 0.03 | 127 | 10 |
| Procyon | +0.01 | 0.01 | 0.01 | 0.00 | 0.00 | +0.05 | –0.06 | 0.02 | 135 | 12 |
| HD 49933 | –0.41 | 0.01 | 0.04 | 0.02 | 0.02 | +0.05 | –0.03 | 0.02 | 93 | 6 |
|
|
||||||||||
| FGK giants | ||||||||||
| Arcturus | –0.52 | 0.01 | 0.00 | 0.00 | 0.06 | +0.01 | +0.02 | 0.04 | 151 | 10 |
| HD 220009 | –0.74 | 0.01 | 0.01 | 0.00 | 0.07 | +0.01 | +0.10 | 0.03 | 148 | 11 |
| μ Leo | +0.25 | 0.02 | 0.00 | 0.00 | 0.13 | –0.01 | +0.01 | 0.08 | 139 | 11 |
| HD 107328 | –0.33 | 0.01 | 0.01 | 0.00 | 0.16 | +0.01 | +0.02 | 0.03 | 137 | 11 |
| β Gem | +0.13 | 0.01 | 0.01 | 0.00 | 0.13 | +0.01 | +0.09 | 0.03 | 146 | 13 |
| ϵ Vir | +0.15 | 0.01 | 0.02 | 0.00 | 0.15 | +0.02 | –0.03 | 0.03 | 139 | 12 |
| ξ Hya | +0.16 | 0.01 | 0.01 | 0.00 | 0.17 | +0.02 | +0.10 | 0.03 | 151 | 11 |
|
|
||||||||||
| M giants | ||||||||||
| ψ Phe | –1.24 | 0.24 | 0.05 | 0.03 | 0.30 | –0.01 | – | – | 23 | 0 |
| α Cet | –0.45 | 0.05 | 0.17 | 0.08 | 0.34 | +0.00 | –0.20 | 0.17 | 35 | 3 |
| γ Sge | –0.17 | 0.04 | 0.13 | 0.09 | 0.22 | –0.01 | –0.25 | 0.12 | 29 | 4 |
| α Tau | –0.37 | 0.02 | 0.02 | 0.02 | 0.12 | +0.00 | +0.06 | 0.10 | 76 | 9 |
| β Ara | –0.05 | 0.04 | 0.01 | 0.04 | 0.16 | +0.00 | –0.34 | 0.08 | 62 | 8 |
|
|
||||||||||
| K dwarfs | ||||||||||
| 61 Cyg B | –0.38 | 0.03 | 0.01 | 0.01 | 0.01 | +0.00 | – | – | 119 | 2 |
| 61 Cyg A | –0.33 | 0.02 | 0.00 | 0.01 | 0.00 | +0.00 | –0.29 | 0.25 | 138 | 3 |
| Gmb 1830 | –1.46 | 0.01 | 0.05 | 0.03 | 0.30 | +0.00 | –0.22 | 0.10 | 116 | 4 |
| ϵ Eri | –0.09 | 0.01 | 0.00 | 0.00 | 0.00 | +0.01 | –0.05 | 0.02 | 153 | 11 |
Notes. The metallicity is associated with different sources or errors: standard deviation of the line-by-line abundance of the selected Fe i lines (σFe i); errors due to the uncertainty in Teff, log g and vmic, (Δ (Teff), Δ (log g), Δ (vmic), respectively); error due to difference between NLTE and LTE Fe i abundance (Δ (LTE) ); error due to difference between Fe i and Fe ii abundance Δ (ion); and standard deviation of the line-by-line mean of Fe ii abundance (σFe ii). The last two columns indicate the number of selected lines used for the determination of Fe i and Fe ii abundances, respectively.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.