Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -1.98 | 1 | 6.57 |
O I | ... | <-0.57 | <2.41 | <8.30 |
Na I | ... | -3.17+-0.12 | -0.19+-0.12 | 3.16+-0.12 |
Mg I | ... | -2.62+-0.17 | 0.36+-0.17 | 4.96+-0.17 |
Al I | ... | -3.31 | -0.33 | 3.16 |
Si I | ... | -2.70+-0.49 | 0.28+-0.49 | 4.85+-0.49 |
Ca I | ... | -2.47+-0.24 | 0.51+-0.24 | 3.89+-0.24 |
Sc II | ... | -2.91+-0.19 | 0.07+-0.19 | 0.26+-0.19 |
Ti I | ... | <-1.99 | <0.99 | <3.03 |
Ti II | ... | -2.64+-0.12 | 0.34+-0.12 | 2.38+-0.12 |
Cr I | ... | -3.17+-0.17 | -0.19+-0.17 | 2.50+-0.17 |
Mn I | ... | -3.58 | -0.6 | 1.81 |
Fe I | ... | -2.98+-0.15 | ... | 4.52+-0.15 |
Fe II | ... | -3.08+-0.11 | -0.1+-0.11 | 4.42+-0.11 |
Co I | ... | -2.61 | 0.37 | 2.31 |
Ni I | ... | -3.33 | -0.35 | 2.92 |
Sr II | ... | -3.46+-0.18 | -0.48+-0.18 | -0.49+-0.18 |
Ba II | ... | -3.22 | -0.24 | -1.09 |
Eu II | ... | <-1.59 | <1.39 | <-1.08 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)