Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.86-0.2 | +-0.2 | 1.83 |
CH | ... | -2.34+-0.25 | 0.52+-0.25 | 6.05 |
NH | ... | <-1.77 | <1.09 | <6.2 |
O I | ... | -2.56+-0.23 | 0.3+-0.23 | 6.13 |
Na I | ... | -2.91+-0.31 | -0.05+-0.31 | 3.33 |
Mg I | ... | -2.37+-0.22 | 0.49+-0.22 | 5.23 |
Al I | ... | -3.63+-0.29 | -0.77+-0.29 | 2.82 |
Si I | ... | -2.15+-0.36 | 0.71+-0.36 | 5.36 |
Ca I | ... | -2.40+-0.22 | 0.46+-0.22 | 3.95 |
Sc II | ... | -2.88+-0.15 | -0.02+-0.15 | 0.23 |
Ti I | ... | -2.39+-0.21 | 0.47+-0.21 | 2.57 |
Ti II | ... | -2.58+-0.14 | 0.28+-0.14 | 2.33 |
V I | ... | <-2.40 | <0.46 | <1.6 |
V II | ... | <-2.46 | <0.40 | <1.54 |
Cr I | ... | -3.06+-0.21 | -0.2+-0.21 | 2.58 |
Mn I | ... | -3.27+-0.2 | -0.41+-0.2 | 2.17 |
Mn II | ... | -3.21+-0.22 | -0.35+-0.22 | 2.18 |
Fe I | ... | -2.86+-0.21 | ... | 4.64 |
Fe II | ... | -2.9+-0.15 | ... | 4.6 |
Co I | ... | -2.68+-0.24 | 0.18+-0.24 | 2.31 |
Ni I | ... | -2.86+-0.28 | 0.00+-0.28 | 3.36 |
Zn I | ... | <-2.16 | <0.70 | <2.44 |
Rb I | ... | <-0.08 | <2.78 | <2.52 |
Sr II | ... | -3.14+-0.2 | -0.28+-0.2 | -0.3 |
Y II | ... | <-3.25 | <-0.39 | <-1.01 |
Zr II | ... | <-2.09 | <0.77 | <0.51 |
Nb II | ... | <-0.02 | <2.84 | <1.4 |
Mo I | ... | <-0.99 | <1.87 | <0.93 |
Tc I | ... | <1.36 | <4.22 | <1.36 |
Ba II | ... | -3.36+-0.14 | -0.5+-0.14 | -1.22 |
Ce II | ... | <-1.69 | <1.17 | <-0.11 |
Pr II | ... | <-1.21 | <1.65 | <-0.5 |
Nd II | ... | <-1.73 | <1.13 | <-0.23 |
Sm II | ... | <-1.15 | <1.71 | <-0.14 |
Eu II | ... | <-1.94 | <0.92 | <-1.43 |
Gd II | ... | <-0.96 | <1.90 | <0.16 |
Tb II | ... | <-0.23 | <2.63 | <-0.33 |
Dy II | ... | <-1.66 | <1.20 | <-0.52 |
Ho II | ... | <-0.85 | <2.01 | <-0.59 |
Er II | ... | <-1.18 | <1.68 | <-0.25 |
Tm II | ... | <-0.63 | <2.23 | <-0.63 |
Yb II | ... | <-2.41 | <0.45 | <-1.33 |
Hf II | ... | <-0.36 | <2.50 | <0.52 |
Pb I | ... | <-0.37 | <2.49 | <1.58 |
Th II | ... | <-0.50 | <2.36 | <-0.5 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)