Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -0.46 | 6.84 | 0.7 |
CH | ... | -2.4+-0.2 | 4.90+-0.2 | 6.15+-0.2 |
NH | ... | <-3.5 | <3.80 | <4.47 |
O I | ... | <-2.3 | <5.00 | <6.57 |
Na I | ... | <-5.5 | <1.80 | <0.83 |
Mg I | ... | -4.3+-0.1 | 3.00+-0.1 | 3.28+-0.1 |
Al I | ... | <-6.2 | <1.10 | <0.27 |
Si I | ... | <-4.3 | <3.00 | <3.25 |
Ca II | ... | -7.2+-0.1 | 0.10+-0.1 | -0.84+-0.1 |
Sc II | ... | <-5.0 | <2.30 | <-1.83 |
Ti II | ... | <-6.3 | <1.00 | <-1.28 |
V II | ... | <-3.3 | <4.00 | <0.70 |
Cr I | ... | <-6.3 | <1.00 | <-0.63 |
Mn I | ... | <-5.8 | <1.50 | <-0.41 |
Fe I | ... | <-7.3 | ... | <0.20 |
Co I | ... | <-4.9 | <2.40 | <0.02 |
Ni I | ... | <-6.4 | <0.90 | <-0.15 |
Cu I | ... | <-3.5 | <3.80 | <0.71 |
Zn I | ... | <-3.4 | <3.90 | <1.20 |
Sr II | ... | <-6.7 | <0.60 | <-3.83 |
Ba II | ... | <-6.1 | <1.20 | <-3.92 |
Eu II | ... | <-2.9 | <4.40 | <-2.39 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)