Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.68-0.2 | +-0.2 | 2.19 |
CH | ... | <-2.35 | <0.33 | <6.2 |
CN | ... | <-0.02 | <2.66 | <7.95 |
O I | ... | -2.10+-0.2 | 0.58+-0.2 | 6.59 |
Mg I | ... | -2.43+-0.21 | 0.25+-0.21 | 5.17 |
Al I | ... | -3.54+-0.26 | -0.86+-0.26 | 2.91 |
Si I | ... | -2.36+-0.36 | 0.32+-0.36 | 5.15 |
Ca I | ... | -2.22+-0.22 | 0.46+-0.22 | 4.12 |
Sc II | ... | -2.73+-0.14 | -0.05+-0.14 | 0.64 |
Ti I | ... | -2.32+-0.21 | 0.36+-0.21 | 2.62 |
Ti II | ... | -2.41+-0.14 | 0.27+-0.14 | 2.76 |
V II | ... | <-2.34 | <0.34 | <1.66 |
Cr I | ... | -2.79+-0.2 | -0.11+-0.2 | 2.84 |
Cr II | ... | -2.65+-0.16 | 0.03+-0.16 | 3.2 |
Mn I | ... | -3.15+-0.2 | -0.47+-0.2 | 2.28 |
Mn II | ... | -3.23+-0.2 | -0.55+-0.2 | 2.41 |
Fe I | ... | -2.68+-0.21 | ... | 4.82 |
Fe II | ... | -2.47+-0.15 | ... | 5.03 |
Co I | ... | -2.71+-0.24 | -0.03+-0.24 | 2.28 |
Ni I | ... | -2.78+-0.24 | -0.1+-0.24 | 3.43 |
Zn I | ... | <-2.02 | <0.66 | <2.58 |
Rb I | ... | <0.20 | <2.88 | <2.8 |
Sr II | ... | -2.50+-0.24 | 0.18+-0.24 | 0.58 |
Y II | ... | -2.89+-0.18 | -0.21+-0.18 | -0.47 |
Zr II | ... | -2.44+-0.17 | 0.24+-0.17 | 0.35 |
Nb II | ... | <0.25 | <2.93 | <1.67 |
Mo I | ... | <-0.72 | <1.96 | <1.2 |
Tc I | ... | <1.41 | <4.09 | <1.41 |
Ba II | ... | -3.00+-0.15 | -0.32+-0.15 | -0.61 |
Ce II | ... | <-1.44 | <1.24 | <0.14 |
Pr II | ... | <-0.87 | <1.81 | <-0.16 |
Nd II | ... | <-1.52 | <1.16 | <-0.02 |
Sm II | ... | <-1.14 | <1.54 | <-0.13 |
Eu II | ... | <-1.64 | <1.04 | <-1.13 |
Gd II | ... | <-0.71 | <1.97 | <0.41 |
Tb II | ... | <-0.03 | <2.65 | <-0.13 |
Dy II | ... | <-1.30 | <1.38 | <-0.16 |
Er II | ... | <-0.89 | <1.79 | <0.04 |
Tm II | ... | <-0.46 | <2.22 | <-0.46 |
Yb II | ... | <-1.86 | <0.82 | <-0.78 |
Hf II | ... | <-0.20 | <2.48 | <0.68 |
Pb I | ... | <-0.20 | <2.48 | <1.75 |
Th II | ... | <-0.10 | <2.58 | <-0.1 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)