| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -3.30 | -0.35 | 5.25 |
| Mg I | ... | -2.73+-0.02 | 0.22+-0.02 | 4.85+-0.02 |
| Al I | ... | -3.28 | -0.33 | 3.19 |
| Si I | ... | -2.71 | 0.24 | 4.84 |
| Ca I | ... | -3.00+-0.08 | -0.05+-0.08 | 3.36+-0.08 |
| Sc II | ... | -2.77+-0.1 | 0.18+-0.1 | 0.40+-0.1 |
| Ti I | ... | -2.95+-0.1 | 0.00+-0.10 | 2.07+-0.1 |
| Ti II | ... | -2.75+-0.13 | 0.2+-0.13 | 2.27+-0.13 |
| V I | ... | -3.16 | -0.21 | 0.84 |
| Cr I | ... | -3.40+-0.25 | -0.45+-0.25 | 2.27+-0.25 |
| Mn I | ... | -3.69+-0.2 | -0.74+-0.2 | 1.70+-0.2 |
| Fe I | ... | -2.95+-0.18 | ... | 4.55+-0.18 |
| Fe II | ... | -2.94+-0.12 | 0.01+-0.12 | 4.56+-0.12 |
| Co I | ... | -2.83+-0.17 | 0.12+-0.17 | 2.09+-0.17 |
| Ni I | ... | -3.13+-0.11 | -0.18+-0.11 | 3.12+-0.11 |
| Zn I | ... | -2.81 | 0.14 | 1.79 |
| Sr II | ... | -5.10+-0.09 | -2.15+-0.09 | -2.13+-0.09 |
| Zr II | ... | <-2.82 | <0.13 | <-0.22 |
| Ba II | ... | -4.87 | -1.92 | -2.74 |
| Ce II | ... | <-2.48 | <0.47 | <-0.90 |
| Eu II | ... | <-3.18 | <-0.23 | <-2.67 |
| Pb I | ... | <-1.49 | <1.46 | <0.46 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
