| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -0.89 | 1.7 | 7.66 |
| Na I | ... | -2.28+-0.15 | 0.31+-0.15 | 4.05+-0.15 |
| Mg I | ... | -2.04+-0.04 | 0.55+-0.04 | 5.54+-0.04 |
| Si I | ... | -0.89+-0.3 | 1.7+-0.3 | 6.66+-0.3 |
| K I | ... | -1.50 | 1.09 | 3.62 |
| Ca I | ... | -1.90+-0.21 | 0.69+-0.21 | 4.46+-0.21 |
| Sc II | ... | -2.06 | 0.53 | 1.11 |
| Ti I | ... | -1.86+-0.14 | 0.73+-0.14 | 3.16+-0.14 |
| Ti II | ... | -1.77+-0.29 | 0.82+-0.29 | 3.25+-0.29 |
| Cr I | ... | -2.97 | -0.38 | 2.70 |
| Fe I | ... | -2.59+-0.2 | ... | 4.91+-0.2 |
| Fe II | ... | -2.57+-0.3 | 0.02+-0.3 | 4.93+-0.3 |
| Y II | ... | -1.81+-0.15 | 0.78+-0.15 | 0.43+-0.15 |
| Ba II | ... | -0.67+-0.16 | 1.92+-0.16 | 1.46+-0.16 |
| La II | ... | -0.94+-0.17 | 1.65+-0.17 | 0.23+-0.17 |
| Ce II | ... | -0.85+-0.02 | 1.74+-0.02 | 0.73+-0.02 |
| Nd II | ... | -0.70+-0.18 | 1.89+-0.18 | 0.80+-0.18 |
| Eu II | ... | <-0.94 | <1.65 | <-0.43 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
