| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -1.09 | 1.82 | 7.46 |
| Na I | ... | -2.67+-0.16 | 0.24+-0.16 | 3.66+-0.16 |
| Mg I | ... | -2.42+-0.2 | 0.49+-0.2 | 5.16+-0.2 |
| Al I | ... | -2.63 | 0.28 | 3.84 |
| K I | ... | -2.31 | 0.6 | 2.81 |
| Ca I | ... | -2.44+-0.04 | 0.47+-0.04 | 3.92+-0.04 |
| Sc II | ... | -2.92 | -0.01 | 0.25 |
| Ti I | ... | -2.52+-0.07 | 0.39+-0.07 | 2.50+-0.07 |
| Ti II | ... | -2.91 | 0.00 | 2.11 |
| Cr I | ... | -3.01+-0.23 | -0.1+-0.23 | 2.66+-0.23 |
| Mn I | ... | -3.21 | -0.3 | 2.18 |
| Fe I | ... | -2.91+-0.16 | ... | 4.59+-0.16 |
| Fe II | ... | -2.93+-0.09 | -0.02+-0.09 | 4.57+-0.09 |
| Sr II | ... | -2.85 | 0.06 | 0.12 |
| Y II | ... | -2.65+-0.13 | 0.26+-0.13 | -0.41+-0.13 |
| Ba II | ... | -1.38+-0.15 | 1.53+-0.15 | 0.75+-0.15 |
| La II | ... | -1.70+-0.2 | 1.21+-0.2 | -0.53+-0.2 |
| Ce II | ... | -1.40 | 1.51 | 0.18 |
| Pr II | ... | -1.08 | 1.83 | -0.37 |
| Nd II | ... | -1.57+-0.15 | 1.34+-0.15 | -0.07+-0.15 |
| Eu II | ... | -2.21 | 0.7 | -1.70 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
