Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.22-0.14 | +-0.14 | 0.79 |
CH | ... | -3.12+-0.25 | 0.1+-0.25 | 5.33 |
NH | ... | -3.37+-0.36 | -0.15+-0.36 | 4.48 |
Mg I | ... | -2.68+-0.15 | 0.54+-0.15 | 4.92 |
Al I | ... | -3.78+-0.3 | -0.56+-0.3 | 2.67 |
Ca I | ... | -2.74+-0.17 | 0.48+-0.17 | 3.6 |
Sc II | ... | -3.25+-0.15 | -0.03+-0.15 | -0.07 |
Ti I | ... | -3.05+-0.14 | 0.17+-0.14 | 1.9 |
Ti II | ... | -2.98+-0.15 | 0.24+-0.15 | 2 |
V I | ... | -3.33+-0.17 | -0.11+-0.17 | 0.6 |
V II | ... | -3.24+-0.24 | -0.02+-0.24 | 0.72 |
Cr I | ... | -3.45+-0.15 | -0.23+-0.15 | 2.19 |
Cr II | ... | -3.14+-0.16 | 0.08+-0.16 | 2.53 |
Mn I | ... | -3.60+-0.16 | -0.38+-0.16 | 1.83 |
Fe I | ... | -3.22+-0.14 | ... | 4.28 |
Fe II | ... | -3.19+-0.15 | ... | 4.31 |
Co I | ... | -3.31+-0.19 | -0.09+-0.19 | 1.67 |
Ni I | ... | -3.16+-0.19 | 0.06+-0.19 | 3.06 |
Cu I | ... | <-3.41 | <-0.19 | <0.8 |
Zn I | ... | -2.69+-0.14 | 0.53+-0.14 | 1.86 |
Sr II | ... | -3.39+-0.25 | -0.17+-0.25 | -0.5 |
Y II | ... | -3.91+-0.18 | -0.69+-0.18 | -1.68 |
Zr II | ... | -3.21+-0.16 | 0.01+-0.16 | -0.6 |
Nb II | ... | <-1.31 | <1.91 | <0.11 |
Mo I | ... | <-2.29 | <0.93 | <-0.37 |
Tc I | ... | <-0.21 | <3.01 | <-0.21 |
Sn I | ... | <-0.85 | <2.37 | <1.15 |
Ba II | ... | -3.60+-0.15 | -0.38+-0.15 | -1.39 |
La II | ... | -3.19+-0.17 | 0.03+-0.17 | -2.07 |
Ce II | ... | <-2.92 | <0.30 | <-1.34 |
Pr II | ... | -2.79+-0.19 | 0.43+-0.19 | -2.04 |
Nd II | ... | -3.09+-0.19 | 0.13+-0.19 | -1.65 |
Sm II | ... | <-2.81 | <0.41 | <-1.8 |
Eu II | ... | -2.94+-0.16 | 0.28+-0.16 | -2.39 |
Gd II | ... | <-2.54 | <0.68 | <-1.42 |
Tb II | ... | <-1.78 | <1.44 | <-1.88 |
Dy II | ... | -2.94+-0.16 | 0.28+-0.16 | -1.81 |
Tm II | ... | <-2.12 | <1.10 | <-2.12 |
Yb II | ... | -3.08+-0.19 | 0.14+-0.19 | -2.13 |
Hf II | ... | <-2.26 | <0.96 | <-1.38 |
Ir I | ... | <-1.82 | <1.40 | <-0.47 |
Pb I | ... | <-1.80 | <1.42 | <0.15 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)