Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.01-0.2 | +-0.2 | 1.88 |
CH | ... | -2.31+-0.25 | 0.7+-0.25 | 6.25 |
NH | ... | <-1.67 | <1.34 | <6.3 |
Mg I | ... | -3.08+-0.3 | -0.07+-0.3 | 4.53 |
Al I | ... | -4.04+-0.21 | -1.03+-0.21 | 2.41 |
Si I | ... | -2.72+-0.36 | 0.29+-0.36 | 4.79 |
Ca I | ... | -2.60+-0.23 | 0.41+-0.23 | 3.74 |
Sc II | ... | -3.22+-0.15 | -0.21+-0.15 | 0.07 |
Ti I | ... | -2.63+-0.22 | 0.38+-0.22 | 2.32 |
Ti II | ... | -2.98+-0.13 | 0.03+-0.13 | 2.1 |
V II | ... | <-2.17 | <0.84 | <1.83 |
Cr I | ... | -3.14+-0.2 | -0.13+-0.2 | 2.5 |
Mn I | ... | -3.78+-0.21 | -0.77+-0.21 | 1.65 |
Fe I | ... | -3.01+-0.21 | ... | 4.49 |
Fe II | ... | -2.87+-0.15 | ... | 4.63 |
Co I | ... | -3.06+-0.28 | -0.05+-0.28 | 1.93 |
Ni I | ... | -3.25+-0.24 | -0.24+-0.24 | 2.97 |
Ga I | ... | <-1.23 | <1.78 | <1.65 |
Sr II | ... | -4.20+-0.14 | -1.19+-0.14 | -1.2 |
Y II | ... | <-3.10 | <-0.09 | <-0.86 |
Zr II | ... | <-2.20 | <0.81 | <0.4 |
Nb II | ... | <0.02 | <3.03 | <1.44 |
Mo I | ... | <-0.74 | <2.27 | <1.18 |
Tc I | ... | <1.51 | <4.52 | <1.51 |
Ba II | ... | -4.07+-0.17 | -1.06+-0.17 | -1.75 |
La II | ... | <-1.73 | <1.28 | <-0.56 |
Ce II | ... | <-1.52 | <1.49 | <0.06 |
Pr II | ... | <-0.90 | <2.11 | <-0.19 |
Nd II | ... | <-1.38 | <1.63 | <0.12 |
Sm II | ... | <-1.09 | <1.92 | <-0.08 |
Eu II | ... | <-1.76 | <1.25 | <-1.25 |
Gd II | ... | <-0.84 | <2.17 | <0.28 |
Tb II | ... | <-0.15 | <2.86 | <-0.25 |
Dy II | ... | <-1.61 | <1.40 | <-0.47 |
Ho II | ... | <-0.76 | <2.25 | <-0.5 |
Er II | ... | <-0.93 | <2.08 | <0 |
Tm II | ... | <-0.57 | <2.44 | <-0.57 |
Yb II | ... | <-2.12 | <0.89 | <-1.04 |
Hf II | ... | <-0.37 | <2.64 | <0.51 |
Pb I | ... | <-0.17 | <2.84 | <1.78 |
Th II | ... | <-0.14 | <2.87 | <-0.14 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)