| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | -0.26+-0.2 | 2.11+-0.2 | 0.9+-0.2 |
| Be II | ... | -4.09 | -1.72 | <-2.80+-1 |
| CH | ... | -0.40 | 1.97 | 7.96+-0.1 |
| C2 | ... | -0.59+-0.12 | 1.97 | 7.96+-0.12 |
| CN | ... | -1.17+-0.15 | 1.34 | 6.8+-0.15 |
| NH | ... | -1.03 | 1.34 | 6.8+-0.15 |
| OH | ... | -1.10 | 1.27 | 7.6+-0.2 |
| Na I | ... | -1.64 | 0.73 | 4.62+-0.15 |
| Mg I | ... | -1.96 | 0.41 | 5.55+-0.12 |
| Al I | ... | -3.40+-0.1 | -0.99 | 3.07+-0.1 |
| Si I | ... | -2.95 | -0.58 | 4.55+-0.14 |
| Ca I | ... | -2.02 | 0.35 | 4.26+-0.1 |
| Sc II | ... | -1.89 | 0.48 | 1.15+-0.1 |
| Ti I | ... | -2.05 | 0.32 | 2.85+-0.1 |
| Ti II | ... | -2.05 | 0.32 | 2.99+-0.1 |
| V II | ... | -2.44+-0.24 | -0.03 | 1.56+-0.24 |
| Cr I | ... | -2.51+-0.1 | -0.09 | 3.16+-0.1 |
| Mn I | ... | -2.86 | -0.49 | 2.61+-0.25 |
| Mn II | ... | -2.78+-0.12 | -0.49 | 2.61+-0.12 |
| Fe I | ... | -2.37+-0.1 | ... | 5.13+-0.1 |
| Fe II | ... | -2.37+-0.1 | ... | 5.13+-0.1 |
| Co I | ... | -2.51 | -0.14 | 2.36+-0.17 |
| Ni I | ... | -2.25+-0.12 | 0.18 | 4+-0.12 |
| Cu I | ... | -3.54 | -1.17 | 0.7+-0.11 |
| Zn I | ... | -2.12 | 0.25 | 2.5+-0.02 |
| Sr II | ... | -2.55 | -0.18 | 0.32+-0.04 |
| Y II | ... | -2.07 | 0.3 | 0.1+-0.1 |
| Zr II | ... | -1.57 | 0.8 | 0.97+-0.11 |
| Nb II | ... | -1.42+-0.3 | 0.98 | 0.0+-0.3 |
| Ba II | ... | -0.42 | 1.95 | 1.73+-0.17 |
| La II | ... | -0.91+-0.16 | 1.47 | 0.26+-0.16 |
| Ce II | ... | -1.42 | 0.95 | 0.15+-0.12 |
| Pr II | ... | -0.90+-0.13 | 1.44 | -0.19+-0.13 |
| Nd II | ... | -0.80+-0.12 | 1.63 | 0.7+-0.12 |
| Sm II | ... | -1.24 | 1.13 | -0.31+-0.2 |
| Eu II | ... | -0.83 | 1.54 | -0.33+-0.2 |
| Gd II | ... | -1.25 | 1.12 | -0.19+-0.2 |
| Tb II | ... | -1.29 | 1.08 | -0.98+-0.2 |
| Dy II | ... | -1.33+-0.2 | 1.07 | -0.19+-0.2 |
| Er II | ... | -1.15 | 1.22 | -0.23+-0.25 |
| Yb II | ... | -0.51 | 1.86 | 0.4+-0.2 |
| Lu II | ... | -1.15 | 1.22 | -1.07+-0.2 |
| Hf II | ... | -0.61 | 1.76 | 0.09+-0.11 |
| Pb I | ... | -0.07 | 2.3 | 1.96+-0.2 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)