| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -0.95 | 1.79 | 7.60 |
| Na I | ... | -2.07+-0.15 | 0.67+-0.15 | 4.26+-0.15 |
| Mg I | ... | -2.28+-0.07 | 0.46+-0.07 | 5.30+-0.07 |
| K I | ... | -2.31 | 0.43 | 2.81 |
| Ca I | ... | -2.58+-0.18 | 0.16+-0.18 | 3.78+-0.18 |
| Ti I | ... | -2.35+-0.1 | 0.39+-0.1 | 2.67+-0.1 |
| Ti II | ... | -2.53+-0.12 | 0.21+-0.12 | 2.49+-0.12 |
| Cr I | ... | -3.17 | -0.43 | 2.50 |
| Fe I | ... | -2.74+-0.15 | ... | 4.76+-0.15 |
| Fe II | ... | -2.66+-0.15 | 0.08+-0.15 | 4.84+-0.15 |
| Sr II | ... | -1.77 | 0.97 | 1.20 |
| Y II | ... | -1.61+-0.29 | 1.13+-0.29 | 0.63+-0.29 |
| Ba II | ... | -1.09+-0.06 | 1.65+-0.06 | 1.04+-0.06 |
| La II | ... | -1.37+-0.04 | 1.37+-0.04 | -0.20+-0.04 |
| Ce II | ... | -1.08 | 1.66 | 0.50 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
