Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.85-0.15 | +-0.15 | 0.92 |
CH | ... | -2.76+-0.25 | 0.09+-0.25 | 5.67 |
NH | ... | -3.10+-0.36 | -0.25+-0.36 | 4.73 |
O I | ... | <-2.33 | <0.52 | <6.54 |
Na I | ... | -3.02+-0.24 | -0.17+-0.24 | 3.22 |
Mg I | ... | -2.45+-0.15 | 0.4+-0.15 | 5.14 |
Al I | ... | -3.65+-0.28 | -0.8+-0.28 | 2.8 |
Si I | ... | -2.20+-0.28 | 0.65+-0.28 | 5.31 |
K I | ... | -2.61+-0.18 | 0.24+-0.18 | 2.42 |
Ca I | ... | -2.48+-0.17 | 0.37+-0.17 | 3.85 |
Sc II | ... | -2.92+-0.14 | -0.07+-0.14 | 0.24 |
Ti I | ... | -2.64+-0.15 | 0.21+-0.15 | 2.31 |
Ti II | ... | -2.61+-0.15 | 0.24+-0.15 | 2.35 |
V I | ... | -2.88+-0.18 | -0.03+-0.18 | 1.05 |
V II | ... | -2.83+-0.25 | 0.02+-0.25 | 1.11 |
Cr I | ... | -3.01+-0.15 | -0.16+-0.15 | 2.63 |
Cr II | ... | -2.72+-0.17 | 0.13+-0.17 | 2.93 |
Mn I | ... | -3.17+-0.15 | -0.32+-0.15 | 2.26 |
Fe I | ... | -2.85+-0.15 | ... | 4.65 |
Fe II | ... | -2.84+-0.16 | ... | 4.66 |
Co I | ... | -2.95+-0.2 | -0.1+-0.2 | 2.04 |
Ni I | ... | -2.82+-0.21 | 0.03+-0.21 | 3.4 |
Cu I | ... | <-2.71 | <0.14 | <1.5 |
Zn I | ... | -2.72+-0.17 | 0.13+-0.17 | 1.83 |
Rb I | ... | <-0.56 | <2.29 | <2.04 |
Sr II | ... | -3.02+-0.25 | -0.17+-0.25 | -0.14 |
Y II | ... | -3.32+-0.2 | -0.47+-0.2 | -1.11 |
Zr II | ... | -2.84+-0.17 | 0.01+-0.17 | -0.26 |
Nb II | ... | <-0.63 | <2.22 | <0.79 |
Mo I | ... | <-1.71 | <1.14 | <0.21 |
Tc I | ... | <0.43 | <3.28 | <0.43 |
Sn I | ... | <-0.17 | <2.68 | <1.83 |
Ba II | ... | -3.31+-0.16 | -0.46+-0.16 | -1.12 |
La II | ... | -2.89+-0.22 | -0.04+-0.22 | -1.78 |
Ce II | ... | <-2.57 | <0.28 | <-0.99 |
Pr II | ... | <-1.96 | <0.89 | <-1.25 |
Nd II | ... | -2.72+-0.2 | 0.13+-0.2 | -1.29 |
Sm II | ... | <-2.07 | <0.78 | <-1.06 |
Eu II | ... | -2.67+-0.18 | 0.18+-0.18 | -2.14 |
Gd II | ... | <-1.72 | <1.13 | <-0.6 |
Tb II | ... | <-1.04 | <1.81 | <-1.14 |
Dy II | ... | <-2.30 | <0.55 | <-1.16 |
Er II | ... | <-2.04 | <0.81 | <-1.11 |
Tm II | ... | <-1.46 | <1.39 | <-1.46 |
Yb II | ... | -2.68+-0.19 | 0.17+-0.19 | -1.75 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)