| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -0.17 | 2.9 | 8.38 |
| Na I | ... | -1.69 | 1.38 | 4.64 |
| Mg I | ... | -2.19+-0.13 | 0.88+-0.13 | 5.39+-0.13 |
| Al I | ... | -3.11 | -0.04 | 3.36 |
| Ca I | ... | -2.67+-0.15 | 0.4+-0.15 | 3.69+-0.15 |
| Sc II | ... | <-1.46 | <1.61 | <1.71 |
| Ti I | ... | <-2.09 | <0.98 | <2.93 |
| Ti II | ... | -2.94+-0.19 | 0.13+-0.19 | 2.08+-0.19 |
| Mn I | ... | -3.40+-0.12 | -0.33+-0.12 | 1.99+-0.12 |
| Fe I | ... | -3.07+-0.17 | ... | 4.43+-0.17 |
| Fe II | ... | -3.21+-0.21 | -0.14+-0.21 | 4.29+-0.21 |
| Co I | ... | -2.30 | 0.77 | 2.62 |
| Ni I | ... | -3.15 | -0.08 | 3.10 |
| Sr II | ... | -2.33 | 0.74 | 0.64 |
| Y II | ... | -2.37+-0.01 | 0.7+-0.01 | -0.13+-0.01 |
| Ba II | ... | -1.79+-0.18 | 1.28+-0.18 | 0.34+-0.18 |
| La II | ... | -1.36+-0.04 | 1.71+-0.04 | -0.19+-0.04 |
| Eu II | ... | <-2.07 | <1 | <-1.56 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
