Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -1.90-0.2 | +-0.2 | 2.08 |
CH | ... | -2.18+-0.25 | -0.28+-0.25 | 6.4 |
Mg I | ... | -1.67+-0.25 | 0.23+-0.25 | 5.93 |
Ca I | ... | -1.53+-0.24 | 0.37+-0.24 | 4.81 |
Sc II | ... | -2.09+-0.16 | -0.19+-0.16 | 1.2 |
Ti I | ... | -1.70+-0.21 | 0.2+-0.21 | 3.25 |
Ti II | ... | -1.72+-0.15 | 0.18+-0.15 | 3.37 |
V I | ... | -2.05+-0.26 | -0.15+-0.26 | 1.88 |
V II | ... | -1.80+-0.29 | 0.1+-0.29 | 2.27 |
Cr I | ... | -2.08+-0.21 | -0.18+-0.21 | 3.56 |
Cr II | ... | -1.65+-0.14 | 0.25+-0.14 | 4.13 |
Mn I | ... | -2.26+-0.23 | -0.36+-0.23 | 3.17 |
Fe I | ... | -1.9+-0.21 | ... | 5.6 |
Fe II | ... | -1.76+-0.14 | ... | 5.74 |
Co I | ... | -2.02+-0.27 | -0.12+-0.27 | 2.97 |
Ni I | ... | -1.82+-0.24 | 0.08+-0.24 | 4.4 |
Cu I | ... | <-2.07 | <-0.17 | <2.14 |
Zn I | ... | -1.76+-0.21 | 0.14+-0.21 | 2.8 |
Sr II | ... | -1.86+-0.24 | 0.04+-0.24 | 1.15 |
Zr II | ... | -1.71+-0.23 | 0.19+-0.23 | 1.01 |
Tc I | ... | <1.61 | <3.51 | <1.61 |
Ba II | ... | -2.32+-0.15 | -0.42+-0.15 | -0.14+-0.15 |
La II | ... | <-1.51 | <0.39 | <-0.34 |
Ce II | ... | <-1.35 | <0.55 | <0.23 |
Pr II | ... | <-0.25 | <1.65 | <0.46 |
Nd II | ... | <-1.03 | <0.87 | <0.47 |
Sm II | ... | <-0.98 | <0.92 | <0.03 |
Eu II | ... | <-1.43 | <0.47 | <-0.92 |
Gd II | ... | <-0.38 | <1.52 | <0.74 |
Tb II | ... | <0.47 | <2.37 | <0.37 |
Dy II | ... | <-0.07 | <1.83 | <1.07 |
Tm II | ... | <0.57 | <2.47 | <0.57 |
Hf II | ... | <-0.11 | <1.79 | <0.77 |
Pb I | ... | <-0.17 | <1.73 | <1.78 |
Th II | ... | <0.76 | <2.66 | <0.76 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)