| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -2.73 | -0.06 | 5.82 |
| Na I | ... | -3.42+-0.01 | -0.75+-0.01 | 2.91+-0.01 |
| Mg I | ... | -2.91+-0.12 | -0.24+-0.12 | 4.67+-0.12 |
| Al I | ... | -3.51 | -0.84 | 2.96 |
| Si I | ... | -2.60+-0.15 | 0.07+-0.15 | 4.95+-0.15 |
| K I | ... | -2.36 | 0.31 | 2.76 |
| Ca I | ... | -2.82+-0.1 | -0.15+-0.1 | 3.54+-0.1 |
| Sc II | ... | -3.23+-0.1 | -0.56+-0.1 | -0.06+-0.1 |
| Ti I | ... | -2.81+-0.11 | -0.14+-0.11 | 2.21+-0.11 |
| Ti II | ... | -2.84+-0.15 | -0.17+-0.15 | 2.18+-0.15 |
| Cr I | ... | -3.11+-0.28 | -0.44+-0.28 | 2.56+-0.28 |
| Mn I | ... | -3.63+-0.1 | -0.96+-0.1 | 1.76+-0.1 |
| Fe I | ... | -2.67+-0.2 | ... | 4.83+-0.2 |
| Fe II | ... | -2.76+-0.13 | -0.09+-0.13 | 4.74+-0.13 |
| Co I | ... | -3.09 | -0.42 | 1.83 |
| Ni I | ... | -3.31+-0.14 | -0.64+-0.14 | 2.94+-0.14 |
| Sr II | ... | -3.50+-0.12 | -0.83+-0.12 | -0.53+-0.12 |
| Y II | ... | -3.36 | -0.69 | -1.12 |
| Ba II | ... | -3.61+-0.1 | -0.94+-0.1 | -1.48+-0.1 |
| La II | ... | <-3.22 | <-0.55 | <-2.05 |
| Eu II | ... | <-3.04 | <-0.37 | <-2.53 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
