Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.93-0.15 | +-0.15 | 0.65 |
CH | ... | -3.86+-0.25 | 0.07+-0.25 | 4.7 |
NH | ... | <-2.97 | <0.96 | <5 |
Na I | ... | -3.86+-0.17 | 0.07+-0.17 | 2.38 |
Mg I | ... | -3.48+-0.16 | 0.45+-0.16 | 4.12 |
Al I | ... | -4.74+-0.17 | -0.81+-0.17 | 1.71 |
Si I | ... | -3.11+-0.32 | 0.82+-0.32 | 4.4 |
Ca I | ... | -3.56+-0.18 | 0.37+-0.18 | 2.78 |
Sc II | ... | -4.14+-0.16 | -0.21+-0.16 | -0.86 |
Ti I | ... | -3.60+-0.16 | 0.33+-0.16 | 1.35 |
Ti II | ... | -3.87+-0.15 | 0.06+-0.15 | 1.21 |
V II | ... | <-3.37 | <0.56 | <0.63 |
Cr I | ... | -4.12+-0.15 | -0.19+-0.15 | 1.52 |
Mn I | ... | -4.10+-0.16 | -0.17+-0.16 | 1.33 |
Mn II | ... | -4.17+-0.21 | -0.24+-0.21 | 1.39 |
Fe I | ... | -3.93+-0.15 | ... | 3.57 |
Fe II | ... | -3.8+-0.16 | ... | 3.7 |
Co I | ... | -3.76+-0.19 | 0.17+-0.19 | 1.23 |
Ni I | ... | -3.69+-0.18 | 0.24+-0.18 | 2.53 |
Cu I | ... | <-3.32 | <0.61 | <0.89 |
Zn I | ... | <-2.78 | <1.15 | <1.82 |
Sr II | ... | -5.17+-0.15 | -1.24+-0.15 | -2.17 |
Y II | ... | <-4.36 | <-0.43 | <-2.12 |
Zr II | ... | <-3.53 | <0.40 | <-0.93 |
Mo I | ... | <-2.06 | <1.87 | <-0.14 |
Tc I | ... | <0.21 | <4.14 | <0.21 |
Ba II | ... | -5.61+-0.16 | -1.68+-0.16 | -3.3 |
La II | ... | <-3.33 | <0.60 | <-2.16 |
Ce II | ... | <-2.97 | <0.96 | <-1.39 |
Pr II | ... | <-2.66 | <1.27 | <-1.95 |
Nd II | ... | <-3.08 | <0.85 | <-1.58 |
Sm II | ... | <-2.47 | <1.46 | <-1.46 |
Eu II | ... | <-3.33 | <0.60 | <-2.82 |
Gd II | ... | <-2.21 | <1.72 | <-1.09 |
Tb II | ... | <-1.79 | <2.14 | <-1.89 |
Dy II | ... | <-3.02 | <0.91 | <-1.88 |
Ho II | ... | <-2.34 | <1.59 | <-2.08 |
Er II | ... | <-2.67 | <1.26 | <-1.74 |
Tm II | ... | <-2.10 | <1.83 | <-2.1 |
Yb II | ... | <-3.66 | <0.27 | <-2.58 |
Hf II | ... | <-1.82 | <2.11 | <-0.94 |
Ir I | ... | <-1.34 | <2.59 | <0.01 |
Pb I | ... | <-1.39 | <2.54 | <0.56 |
Th II | ... | <-1.83 | <2.10 | <-1.83 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)