Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.39-0.2 | +-0.2 | 2.28 |
CH | ... | -2.30+-0.25 | 0.09+-0.25 | 6.28 |
NH | ... | <-2.37 | <0.02 | <5.6 |
O I | ... | -2.07+-0.21 | 0.32+-0.21 | 6.62 |
Na I | ... | -2.49+-0.31 | -0.1+-0.31 | 3.75 |
Mg I | ... | -2.09+-0.23 | 0.3+-0.23 | 5.51 |
Al I | ... | -3.13+-0.32 | -0.74+-0.32 | 3.32 |
Si I | ... | -1.89+-0.37 | 0.5+-0.37 | 5.62 |
K I | ... | -2.08+-0.23 | 0.31+-0.23 | 2.95 |
Ca I | ... | -1.93+-0.22 | 0.46+-0.22 | 4.41 |
Sc II | ... | -2.35+-0.15 | 0.04+-0.15 | 0.95 |
Ti I | ... | -2.01+-0.21 | 0.38+-0.21 | 2.94 |
Ti II | ... | -2.01+-0.14 | 0.38+-0.14 | 3.09 |
V I | ... | -2.31+-0.24 | 0.08+-0.24 | 1.62 |
V II | ... | -2.27+-0.26 | 0.12+-0.26 | 1.81 |
Cr I | ... | -2.41+-0.21 | -0.02+-0.21 | 3.23 |
Cr II | ... | -2.27+-0.15 | 0.12+-0.15 | 3.51 |
Mn I | ... | -2.72+-0.21 | -0.33+-0.21 | 2.71 |
Mn II | ... | -2.66+-0.24 | -0.27+-0.24 | 2.92 |
Fe I | ... | -2.39+-0.21 | ... | 5.11 |
Fe II | ... | -2.24+-0.14 | ... | 5.26 |
Co I | ... | -2.35+-0.25 | 0.04+-0.25 | 2.64 |
Ni I | ... | -2.26+-0.27 | 0.13+-0.27 | 3.96 |
Zn I | ... | -2.02+-0.21 | 0.37+-0.21 | 2.54 |
Rb I | ... | <-0.18 | <2.21 | <2.42 |
Sr II | ... | -2.14+-0.24 | 0.25+-0.24 | 0.87 |
Y II | ... | -2.70+-0.18 | -0.31+-0.18 | -0.34 |
Zr II | ... | -2.23+-0.17 | 0.16+-0.17 | 0.5 |
Nb II | ... | <-0.29 | <2.10 | <1.13 |
Tc I | ... | <1.14 | <3.53 | <1.14 |
Ba II | ... | -2.66+-0.14 | -0.27+-0.14 | -0.33 |
La II | ... | -2.30+-0.21 | 0.09+-0.21 | -1.05 |
Ce II | ... | <-1.39 | <1.00 | <0.19 |
Pr II | ... | <-0.91 | <1.48 | <-0.2 |
Nd II | ... | <-1.87 | <0.52 | <-0.37 |
Sm II | ... | <-1.45 | <0.94 | <-0.44 |
Eu II | ... | -2.25+-0.29 | 0.14+-0.29 | -1.59 |
Gd II | ... | <-1.22 | <1.17 | <-0.1 |
Tb II | ... | <-0.23 | <2.16 | <-0.33 |
Dy II | ... | <-1.52 | <0.87 | <-0.38 |
Er II | ... | <-1.28 | <1.11 | <-0.35 |
Tm II | ... | <-0.83 | <1.56 | <-0.83 |
Yb II | ... | -2.57+-0.45 | -0.18+-0.45 | -1.5 |
Hf II | ... | <-0.56 | <1.83 | <0.32 |
Pb I | ... | <-0.43 | <1.96 | <1.52 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)