| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -1.99 | 0.66 | 6.56 |
| Mg I | ... | -2.23+-0.11 | 0.42+-0.11 | 5.35+-0.11 |
| Al I | ... | -2.92+-0.14 | -0.27+-0.14 | 3.55+-0.14 |
| Si I | ... | -2.64 | 0.01 | 4.91 |
| Ca I | ... | -2.23+-0.18 | 0.42+-0.18 | 4.13+-0.18 |
| Sc II | ... | -2.55+-0.07 | 0.1+-0.07 | 0.62+-0.07 |
| Ti I | ... | <-1.82+-0.38 | <0.83+-0.38 | <3.20+-0.38 |
| Ti II | ... | -2.29+-0.16 | 0.36+-0.16 | 2.73+-0.16 |
| Cr I | ... | -3.07+-0.11 | -0.42+-0.11 | 2.60+-0.11 |
| Mn I | ... | -3.52 | -0.87 | 1.87 |
| Fe I | ... | -2.65+-0.14 | ... | 4.85+-0.14 |
| Fe II | ... | -2.58+-0.17 | 0.07+-0.17 | 4.92+-0.17 |
| Co I | ... | -2.55+-0.1 | 0.1+-0.1 | 2.37+-0.1 |
| Ni I | ... | -2.83+-0.18 | -0.18+-0.18 | 3.42+-0.18 |
| Zn I | ... | <-2.14 | <0.51 | <2.46 |
| Sr II | ... | -2.69+-0.04 | -0.04+-0.04 | 0.28+-0.04 |
| Ba II | ... | -2.80 | -0.15 | -0.67 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
