Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | 0.87 | 4.12 | 2.03 |
Mg | ... | -3.00+-0.17 | +0.25+-0.17 | 4.58+-0.17 |
Si | ... | -3.15 | +0.10 | 4.40 |
Ca I | ... | -2.87+-0.11 | +0.38+-0.11 | 3.49+-0.11 |
Ca II | ... | -2.75 | +0.50 | 3.61 |
Sc | ... | -3.06 | +0.19 | 0.11 |
Ti I | ... | -2.16 | +1.09 | 2.86 |
Ti II | ... | -2.73+-0.13 | +0.52+-0.13 | 2.29+-0.13 |
Cr | ... | -3.47+-0.23 | -0.22+-0.23 | 2.20+-0.23 |
Mn | ... | -3.92 | -0.67 | 1.47 |
Fe | ... | -3.25 | ... | 4.25 |
Fe I | ... | -3.25+-0.11 | ... | 4.25+-0.11 |
Fe II | ... | -3.25+-0.05 | ... | 4.25+-0.05 |
Co | ... | -2.76 | +0.49 | 2.16 |
Ni | ... | -3.29+-0.13 | -0.04+-0.13 | 2.96+-0.13 |
Sr | ... | -3.81 | -0.56 | -0.84 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)