| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li | ... | <0.23 | <3.24 | <1.39 |
| Mg | ... | -2.98+-0.2 | +0.03+-0.20 | 4.60+-0.2 |
| Ca I | ... | -2.73+-0.14 | +0.28+-0.14 | 3.63+-0.14 |
| Ca II | ... | -3.07 | -0.06 | 3.29 |
| Sc | ... | -2.52 | +0.49 | 0.65 |
| Ti II | ... | -2.59 | +0.42 | 2.43 |
| Cr | ... | -3.33+-0.17 | -0.32+-0.17 | 2.34+-0.17 |
| Mn | ... | -3.26+-0.16 | -0.25+-0.16 | 2.13+-0.16 |
| Fe | ... | -3.01 | ... | 4.49 |
| Fe I | ... | -3.01+-0.14 | ... | 4.49+-0.14 |
| Fe II | ... | -3.01 | ... | 4.49 |
| Co | ... | -2.37 | +0.64 | 2.55 |
| Ni | ... | -2.72+-0.16 | +0.29+-0.16 | 3.53+-0.16 |
| Sr | ... | -3.79 | -0.78 | -0.82 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
