Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.82-0.2 | +-0.2 | 1.7 |
CH | ... | -2.49+-0.25 | 0.33+-0.25 | 5.86 |
NH | ... | <-2.42 | <0.40 | <5.55 |
O I | ... | <-2.21 | <0.61 | <6.66 |
Mg I | ... | -2.30+-0.22 | 0.52+-0.22 | 5.3 |
Al I | ... | -3.57+-0.31 | -0.75+-0.31 | 2.88 |
Si I | ... | -2.39+-0.36 | 0.43+-0.36 | 5.12 |
K I | ... | -2.49+-0.24 | 0.33+-0.24 | 2.54 |
Ca I | ... | -2.41+-0.22 | 0.41+-0.22 | 3.94 |
Sc II | ... | -2.70+-0.15 | 0.12+-0.15 | 0.37 |
Ti I | ... | -2.41+-0.2 | 0.41+-0.2 | 2.54 |
Ti II | ... | -2.58+-0.14 | 0.24+-0.14 | 2.28 |
V II | ... | -2.42+-0.34 | 0.4+-0.34 | 1.43 |
Cr I | ... | -3.04+-0.2 | -0.22+-0.2 | 2.61 |
Mn I | ... | -3.24+-0.2 | -0.42+-0.2 | 2.19 |
Mn II | ... | -3.20+-0.2 | -0.38+-0.2 | 2.14 |
Fe I | ... | -2.82+-0.21 | ... | 4.68 |
Fe II | ... | -2.9+-0.15 | ... | 4.6 |
Co I | ... | -2.80+-0.25 | 0.02+-0.25 | 2.19 |
Ni I | ... | -2.99+-0.26 | -0.17+-0.26 | 3.24 |
Zn I | ... | <-2.22 | <0.60 | <2.38 |
Sr II | ... | -3.21+-0.18 | -0.39+-0.18 | -0.42 |
Y II | ... | -3.40+-0.19 | -0.58+-0.19 | -1.28 |
Zr II | ... | <-1.86 | <0.96 | <0.74 |
Mo I | ... | <-1.06 | <1.76 | <0.86 |
Tc I | ... | <1.21 | <4.03 | <1.21 |
Ba II | ... | -3.95+-0.15 | -1.13+-0.15 | -1.85 |
La II | ... | <-1.96 | <0.86 | <-0.79 |
Ce II | ... | <-1.71 | <1.11 | <-0.13 |
Pr II | ... | <-1.18 | <1.64 | <-0.47 |
Nd II | ... | <-1.69 | <1.13 | <-0.19 |
Sm II | ... | <-1.22 | <1.60 | <-0.21 |
Eu II | ... | <-1.90 | <0.92 | <-1.39 |
Gd II | ... | <-1.07 | <1.75 | <0.05 |
Tb II | ... | <-0.27 | <2.55 | <-0.37 |
Dy II | ... | <-1.66 | <1.16 | <-0.52 |
Ho II | ... | <-0.96 | <1.86 | <-0.7 |
Er II | ... | <-1.33 | <1.49 | <-0.4 |
Tm II | ... | <-0.68 | <2.14 | <-0.68 |
Yb II | ... | <-2.54 | <0.28 | <-1.46 |
Hf II | ... | <-0.45 | <2.37 | <0.43 |
Pb I | ... | <-0.47 | <2.35 | <1.48 |
Th II | ... | <-0.47 | <2.35 | <-0.47 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)