Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.43-0.22 | +-0.22 | 1.56 |
CH | ... | -2.09+-0.25 | 0.34+-0.25 | 6.35 |
NH | ... | <-1.72 | <0.71 | <6.25 |
O I | ... | -2.25+-0.21 | 0.18+-0.21 | 6.44 |
Mg I | ... | -2.14+-0.22 | 0.29+-0.22 | 5.46 |
Al I | ... | -3.26+-0.31 | -0.83+-0.31 | 3.19 |
Si I | ... | -1.85+-0.29 | 0.58+-0.29 | 5.66 |
Ca I | ... | -2.02+-0.22 | 0.41+-0.22 | 4.32 |
Sc II | ... | -2.34+-0.15 | 0.09+-0.15 | 0.82 |
Ti I | ... | -2.11+-0.22 | 0.32+-0.22 | 2.84 |
Ti II | ... | -2.08+-0.15 | 0.35+-0.15 | 2.88 |
V II | ... | -2.21+-0.31 | 0.22+-0.31 | 1.73 |
Cr I | ... | -2.53+-0.22 | -0.1+-0.22 | 3.1 |
Cr II | ... | -2.20+-0.16 | 0.23+-0.16 | 3.45 |
Mn I | ... | -2.68+-0.21 | -0.25+-0.21 | 2.75 |
Mn II | ... | -2.86+-0.22 | -0.43+-0.22 | 2.59 |
Fe I | ... | -2.43+-0.21 | ... | 5.07 |
Fe II | ... | -2.42+-0.15 | ... | 5.08 |
Co I | ... | -2.37+-0.26 | 0.06+-0.26 | 2.62 |
Ni I | ... | -2.38+-0.27 | 0.05+-0.27 | 3.83 |
Zn I | ... | -2.29+-0.24 | 0.14+-0.24 | 2.27 |
Rb I | ... | <-0.23 | <2.20 | <2.37 |
Sr II | ... | -2.42+-0.23 | 0.01+-0.23 | 0.46 |
Y II | ... | -3.00+-0.23 | -0.57+-0.23 | -0.78 |
Zr II | ... | -2.37+-0.27 | 0.06+-0.27 | 0.22 |
Nb II | ... | <-0.18 | <2.25 | <1.24 |
Mo I | ... | <-0.88 | <1.55 | <1.04 |
Tc I | ... | <1.18 | <3.61 | <1.18 |
Ba II | ... | -2.91+-0.15 | -0.48+-0.15 | -0.72 |
Ce II | ... | <-1.70 | <0.73 | <-0.12 |
Pr II | ... | <-1.06 | <1.37 | <-0.35 |
Nd II | ... | <-1.90 | <0.53 | <-0.4 |
Sm II | ... | <-1.30 | <1.13 | <-0.29 |
Eu II | ... | <-1.39 | <1.04 | <-0.88 |
Gd II | ... | <-1.00 | <1.43 | <0.12 |
Tb II | ... | <-0.30 | <2.13 | <-0.4 |
Dy II | ... | <-1.51 | <0.92 | <-0.37 |
Er II | ... | <-1.21 | <1.22 | <-0.28 |
Tm II | ... | <-0.77 | <1.66 | <-0.77 |
Yb II | ... | -2.31+-0.52 | 0.12+-0.52 | -1.38 |
Hf II | ... | <-0.38 | <2.05 | <0.5 |
Pb I | ... | <-0.55 | <1.88 | <1.4 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)