| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -0.83 | 2.32 | 7.72 |
| Na I | ... | -2.31+-0.12 | 0.84+-0.12 | 4.02+-0.12 |
| Mg I | ... | -2.53+-0.07 | 0.62+-0.07 | 5.05+-0.07 |
| Al I | ... | -3.17 | -0.02 | 3.30 |
| Si I | ... | -3.84 | -0.69 | 3.71 |
| Ca I | ... | -2.81+-0.21 | 0.34+-0.21 | 3.55+-0.21 |
| Ti I | ... | -2.49 | 0.66 | 2.53 |
| Ti II | ... | -2.84+-0.2 | 0.31+-0.2 | 2.18+-0.2 |
| Cr I | ... | -3.28+-0.08 | -0.13+-0.08 | 2.39+-0.08 |
| Mn I | ... | -3.66+-0.04 | -0.51+-0.04 | 1.73+-0.04 |
| Fe I | ... | -3.15+-0.13 | ... | 4.35+-0.13 |
| Fe II | ... | -3.24+-0.04 | -0.09+-0.04 | 4.26+-0.04 |
| Zn I | ... | -2.11 | 1.04 | 2.49 |
| Y II | ... | -1.82 | 1.33 | 0.42 |
| Ba II | ... | -1.87+-0.11 | 1.28+-0.11 | 0.26+-0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
