Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.40-0.2 | +-0.2 | 2.23 |
CH | ... | -2.19+-0.25 | 0.21+-0.25 | 6.37 |
O I | ... | -1.98+-0.2 | 0.42+-0.2 | 6.71 |
Na I | ... | -2.19+-0.33 | 0.21+-0.33 | 4.05 |
Mg I | ... | -2.05+-0.22 | 0.35+-0.22 | 5.56 |
Al I | ... | -3.01+-0.33 | -0.61+-0.33 | 3.44 |
Ca I | ... | -1.91+-0.22 | 0.49+-0.22 | 4.43 |
Sc II | ... | -2.22+-0.13 | 0.18+-0.13 | 1.06 |
Ti I | ... | -1.99+-0.2 | 0.41+-0.2 | 2.96 |
Ti II | ... | -1.98+-0.14 | 0.42+-0.14 | 3.1 |
V II | ... | -2.06+-0.25 | 0.34+-0.25 | 2 |
Cr I | ... | -2.43+-0.2 | -0.03+-0.2 | 3.21 |
Cr II | ... | -2.19+-0.15 | 0.21+-0.15 | 3.58 |
Mn I | ... | -2.75+-0.22 | -0.35+-0.22 | 2.69 |
Fe I | ... | -2.4+-0.2 | ... | 5.1 |
Fe II | ... | -2.27+-0.14 | ... | 5.23 |
Co I | ... | -2.39+-0.22 | 0.01+-0.22 | 2.6 |
Ni I | ... | -2.33+-0.22 | 0.07+-0.22 | 3.89 |
Zn I | ... | -2.13+-0.22 | 0.27+-0.22 | 2.43 |
Rb I | ... | <0.00 | <2.40 | <2.6 |
Sr II | ... | -2.06+-0.24 | 0.34+-0.24 | 0.94 |
Zr II | ... | -1.84+-0.15 | 0.56+-0.15 | 0.87 |
Tc I | ... | <1.74 | <4.14 | <1.74 |
Ba II | ... | -2.25+-0.14 | 0.15+-0.14 | 0.06 |
La II | ... | <-1.65 | <0.75 | <-0.48 |
Ce II | ... | <-1.37 | <1.03 | <0.21 |
Pr II | ... | <-0.91 | <1.49 | <-0.2 |
Nd II | ... | <-1.45 | <0.95 | <0.05 |
Sm II | ... | <-0.89 | <1.51 | <0.12 |
Eu II | ... | <-1.58 | <0.82 | <-1.07 |
Gd II | ... | <-0.71 | <1.69 | <0.41 |
Tb II | ... | <0.60 | <3.00 | <0.5 |
Dy II | ... | <-1.37 | <1.03 | <-0.23 |
Tm II | ... | <0.68 | <3.08 | <0.68 |
Hf II | ... | <-0.37 | <2.03 | <0.51 |
Pb I | ... | <-0.30 | <2.10 | <1.65 |
Th II | ... | <0.21 | <2.61 | <0.21 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)