Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -1.94-0.1 | +-0.1 | 1.92 |
CH | ... | -1.99+-0.25 | -0.05+-0.25 | 6.43 |
Mg I | ... | -1.64+-0.13 | 0.3+-0.13 | 5.95 |
Si I | ... | -1.33+-0.19 | 0.61+-0.19 | 6.18 |
Ca I | ... | -1.60+-0.16 | 0.34+-0.16 | 4.73 |
Sc II | ... | -2.11+-0.15 | -0.17+-0.15 | 1.04 |
Ti I | ... | -1.77+-0.1 | 0.17+-0.1 | 3.17 |
Ti II | ... | -1.66+-0.13 | 0.28+-0.13 | 3.28 |
V I | ... | -2.09+-0.17 | -0.15+-0.17 | 1.84 |
V II | ... | -1.73+-0.3 | 0.21+-0.3 | 2.2 |
Cr I | ... | -2.11+-0.1 | -0.17+-0.1 | 3.53 |
Cr II | ... | -1.67+-0.14 | 0.27+-0.14 | 3.97 |
Mn I | ... | -2.32+-0.11 | -0.38+-0.11 | 3.11 |
Fe I | ... | -1.94+-0.11 | ... | 5.56 |
Fe II | ... | -1.94+-0.14 | ... | 5.56 |
Co I | ... | -2.11+-0.21 | -0.17+-0.21 | 2.88 |
Ni I | ... | -1.89+-0.15 | 0.05+-0.15 | 4.32 |
Cu I | ... | <-2.30 | <-0.36 | <1.91 |
Zn I | ... | -1.82+-0.11 | 0.12+-0.11 | 2.73 |
Sr II | ... | -1.83+-0.14 | 0.11+-0.14 | 1.04 |
Zr II | ... | -1.65+-0.31 | 0.29+-0.31 | 0.93 |
Tc I | ... | <1.59 | <3.53 | <1.59 |
Ba II | ... | -2.07+-0.13 | -0.13+-0.13 | 0.11 |
Ce II | ... | <-1.61 | <0.33 | <-0.03 |
Sm II | ... | <-1.18 | <0.76 | <-0.17 |
Eu II | ... | -1.35+-0.25 | 0.59+-0.25 | -0.83 |
Gd II | ... | <-0.62 | <1.32 | <0.5 |
Tb II | ... | <0.45 | <2.39 | <0.35 |
Dy II | ... | <-0.67 | <1.27 | <0.47 |
Hf II | ... | <0.07 | <2.01 | <0.95 |
Pb I | ... | <0.01 | <1.95 | <1.96 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)