Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | <0.04 | <3.24 | <1.20 |
Mg | ... | -2.90+-0.12 | +0.30+-0.12 | 4.68+-0.12 |
Si | ... | -2.82 | +0.38 | 4.73 |
Ca I | ... | -2.73+-0.16 | +0.47+-0.16 | 3.63+-0.16 |
Ca II | ... | -3.05 | +0.15 | 3.31 |
Sc | ... | -3.09 | +0.11 | 0.08 |
Ti I | ... | -2.43+-0.18 | +0.77+-0.18 | 2.59+-0.18 |
Ti II | ... | -2.77+-0.15 | +0.43+-0.15 | 2.25+-0.15 |
Cr | ... | -3.42+-0.13 | -0.22+-0.13 | 2.25+-0.13 |
Mn | ... | -3.67+-0.05 | -0.47+-0.05 | 1.72+-0.05 |
Fe | ... | -3.20 | ... | 4.30 |
Fe I | ... | -3.20+-0.11 | ... | 4.30+-0.11 |
Fe II | ... | -3.20+-0.03 | ... | 4.30+-0.03 |
Co | ... | -2.76+-0.12 | +0.44+-0.12 | 2.16+-0.12 |
Ni | ... | -3.22+-0.22 | -0.02+-0.22 | 3.03+-0.22 |
Sr | ... | -3.13+-0.07 | +0.07+-0.07 | -0.16+-0.07 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)