Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.63-0.2 | +-0.2 | 1.99 |
CH | ... | <-2.45 | <1.18 | <6.1 |
CN | ... | <0.23 | <3.86 | <8.2 |
O I | ... | <-2.98 | <0.65 | <5.89 |
Na I | ... | -3.73+-0.22 | -0.1+-0.22 | 2.51 |
Mg I | ... | -3.29+-0.22 | 0.34+-0.22 | 4.31 |
Al I | ... | -4.41+-0.23 | -0.78+-0.23 | 2.04 |
Si I | ... | -3.55+-0.26 | 0.08+-0.26 | 3.96 |
Ca I | ... | -3.09+-0.24 | 0.54+-0.24 | 3.25 |
Sc II | ... | -3.63+-0.15 | 0.00+-0.15 | -0.2 |
Ti II | ... | -3.43+-0.14 | 0.2+-0.14 | 1.8 |
V I | ... | <-2.23 | <1.40 | <1.77 |
V II | ... | <-2.21 | <1.42 | <1.79 |
Cr I | ... | -3.74+-0.2 | -0.11+-0.2 | 1.9 |
Mn I | ... | <-4.08 | <-0.45 | <1.31 |
Fe I | ... | -3.63+-0.21 | ... | 3.87 |
Fe II | ... | -3.35+-0.17 | ... | 4.15 |
Co I | ... | <-3.02 | <0.61 | <1.9 |
Ni I | ... | -3.63+-0.33 | 0.00+-0.33 | 2.59 |
Cu I | ... | <-1.91 | <1.72 | <2.3 |
Zn I | ... | <-2.26 | <1.37 | <2.34 |
Ga I | ... | <-1.42 | <2.21 | <1.46 |
Rb I | ... | <0.27 | <3.90 | <2.87 |
Sr II | ... | -5.00+-0.17 | -1.37+-0.17 | -1.85 |
Y II | ... | <-2.42 | <1.21 | <-0.18 |
Zr II | ... | <-2.33 | <1.30 | <0.27 |
Nb II | ... | <0.05 | <3.68 | <1.47 |
Mo I | ... | <-0.78 | <2.85 | <1.14 |
Tc I | ... | <1.45 | <5.08 | <1.45 |
Ba II | ... | <-3.83 | <-0.20 | <-1.7 |
La II | ... | <-1.94 | <1.69 | <-0.77 |
Ce II | ... | <-1.58 | <2.05 | <0 |
Pr II | ... | <-1.04 | <2.59 | <-0.33 |
Nd II | ... | <-1.64 | <1.99 | <-0.14 |
Sm II | ... | <-1.12 | <2.51 | <-0.11 |
Eu II | ... | <-1.78 | <1.85 | <-1.27 |
Gd II | ... | <-0.92 | <2.71 | <0.2 |
Tb II | ... | <-0.27 | <3.36 | <-0.37 |
Dy II | ... | <-1.44 | <2.19 | <-0.3 |
Ho II | ... | <-0.73 | <2.90 | <-0.47 |
Er II | ... | <-1.08 | <2.55 | <-0.15 |
Tm II | ... | <-0.66 | <2.97 | <-0.66 |
Yb II | ... | <-2.18 | <1.45 | <-1.1 |
Hf II | ... | <-0.28 | <3.35 | <0.6 |
Pb I | ... | <-0.41 | <3.22 | <1.54 |
Th II | ... | <-0.28 | <3.35 | <-0.28 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)