Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.51-0.2 | +-0.2 | 2.2 |
CH | ... | -2.41+-0.25 | 0.1+-0.25 | 6.18 |
NH | ... | <-0.97 | <1.54 | <7 |
O I | ... | -1.96+-0.2 | 0.55+-0.2 | 6.73 |
Na I | ... | -2.71+-0.28 | -0.2+-0.28 | 3.52 |
Mg I | ... | -2.25+-0.22 | 0.26+-0.22 | 5.35 |
Al I | ... | -3.33+-0.3 | -0.82+-0.3 | 3.11 |
Si I | ... | -2.14+-0.36 | 0.37+-0.36 | 5.37 |
Ca I | ... | -2.06+-0.22 | 0.45+-0.22 | 4.28 |
Sc II | ... | -2.48+-0.15 | 0.03+-0.15 | 0.83 |
Ti I | ... | -2.16+-0.2 | 0.35+-0.2 | 2.79 |
Ti II | ... | -2.19+-0.14 | 0.32+-0.14 | 2.92 |
V II | ... | -2.02+-0.24 | 0.49+-0.24 | 2.07 |
Cr I | ... | -2.64+-0.22 | -0.13+-0.22 | 2.99 |
Cr II | ... | -2.27+-0.15 | 0.24+-0.15 | 3.53 |
Mn I | ... | -2.83+-0.21 | -0.32+-0.21 | 2.6 |
Mn II | ... | -2.90+-0.2 | -0.39+-0.2 | 2.69 |
Fe I | ... | -2.51+-0.21 | ... | 4.99 |
Fe II | ... | -2.35+-0.14 | ... | 5.15 |
Co I | ... | -2.47+-0.24 | 0.04+-0.24 | 2.51 |
Ni I | ... | -2.38+-0.28 | 0.13+-0.28 | 3.84 |
Zn I | ... | <-2.17 | <0.34 | <2.43 |
Rb I | ... | <0.27 | <2.78 | <2.87 |
Sr II | ... | -2.34+-0.24 | 0.17+-0.24 | 0.69 |
Y II | ... | -2.80+-0.18 | -0.29+-0.18 | -0.43 |
Zr II | ... | -2.22+-0.18 | 0.29+-0.18 | 0.52 |
Mo I | ... | <-0.53 | <1.98 | <1.39 |
Tc I | ... | <1.67 | <4.18 | <1.67 |
Ba II | ... | -2.84+-0.14 | -0.33+-0.14 | -0.5 |
Ce II | ... | <-1.29 | <1.22 | <0.29 |
Pr II | ... | <-0.89 | <1.62 | <-0.18 |
Nd II | ... | <-1.48 | <1.03 | <0.02 |
Sm II | ... | <-1.10 | <1.41 | <-0.09 |
Eu II | ... | -1.88+-0.16 | 0.63+-0.16 | -1.2 |
Gd II | ... | <-0.79 | <1.72 | <0.33 |
Tb II | ... | <-0.01 | <2.50 | <-0.11 |
Dy II | ... | <-1.42 | <1.09 | <-0.28 |
Ho II | ... | <-0.24 | <2.27 | <0.02 |
Er II | ... | <-0.95 | <1.56 | <-0.02 |
Tm II | ... | <-0.49 | <2.02 | <-0.49 |
Yb II | ... | -2.27+-0.2 | 0.24+-0.2 | -1.19 |
Hf II | ... | <-0.23 | <2.28 | <0.65 |
Pb I | ... | <-0.13 | <2.38 | <1.82 |
Th II | ... | <-0.15 | <2.36 | <-0.15 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)