| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | <0.24 | <3.46 | <1.4 |
| Mg I | ... | -3.27+-0.11 | -0.05+-0.11 | 4.31+-0.11 |
| Al I | ... | -4.27+-0.19 | -1.05+-0.19 | 2.20+-0.19 |
| Si I | ... | -3.04 | 0.18 | 4.51 |
| Ca I | ... | -3.08+-0.22 | 0.14+-0.22 | 3.28+-0.22 |
| Ca II | ... | -2.75+-0.26 | 0.47+-0.26 | 3.61+-0.26 |
| Ti II | ... | -2.68+-0.05 | 0.54+-0.05 | 2.34+-0.05 |
| Cr I | ... | -3.38 | -0.16 | 2.29 |
| Fe I | ... | -3.22+-0.24 | ... | 4.28+-0.24 |
| Fe II | ... | -3.11+-0.01 | ... | 4.39+-0.01 |
| Co I | ... | -2.28 | 0.94 | 2.64 |
| Ni I | ... | -2.95+-0.21 | 0.27+-0.21 | 3.30+-0.21 |
| Sr II | ... | -3.71 | -0.49 | -0.74 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
