Table 3.
Non-LTE corrections of abundances.
| Elem. | Ref. | G112-43 | G112-44 | Comp.stars | Difference (a) |
|---|---|---|---|---|---|
| δ[X/H] | δ[X/H] | ⟨δ[X/H]⟩ | ⟨δ[X/Fe]⟩ | ||
| Fe I | 1 | +0.109 | +0.088 | +0.082 | ... |
| C I | 2 | −0.035 | −0.037 | −0.035 | −0.017 |
| O I | 2 | −0.012 | ... | +0.074 | −0.113 |
| Na I | 3 | +0.016 | +0.024 | +0.029 | −0.025 |
| Mg I | 4 | +0.040 | +0.017 | +0.014 | −0.002 |
| Si I | 5 | −0.004 | +0.000 | +0.000 | −0.018 |
| Ca I | 6 | +0.062 | +0.048 | +0.042 | −0.003 |
| Ti I | 7 | +0.216 | +0.192 | +0.176 | +0.012 |
| Cr I | 8 | +0.179 | +0.162 | +0.152 | +0.002 |
| Mn I | 9 | +0.230 | +0.226 | +0.214 | −0.002 |
| Cu I | 10 | +0.160 | +0.100 | +0.100 | +0.014 |
| Zn I | 11 | +0.125 | +0.096 | +0.087 | +0.007 |
| Ba II | 12 | +0.042 | +0.024 | +0.024 | −0.007 |
Notes.
Difference between the mean non-LTE correction of [X/Fe] for G 112-43/44 and the comparison stars. While Cols. 3, 4, and 5 refer to non-LTE corrections of [X/H], Col. 6 gives the corrections of [X/Fe].
References. (1) Amarsi et al. (2016); (2) Amarsi et al. (2019); (3) Lind et al. (2011), (4) Bergemann et al. (2017); (5) Bergemann et al. (2013); (6) Mashonkina et al. (2017); (7) Bergemann (2011); (8) Bergemann & Cescutti (2010); (9) Bergemann & Gehren (2008); (10) Yan et al. (2016); (11) Takeda et al. (2005); (12) Korotin et al. (2015).
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