Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.55-0.2 | +-0.2 | 1.66 |
CH | ... | <-2.90 | <0.65 | <5.65 |
NH | ... | <-2.26 | <1.29 | <5.71 |
O I | ... | <-1.64 | <1.91 | <7.23 |
Na I | ... | -3.71+-0.22 | -0.16+-0.22 | 2.53 |
Mg I | ... | -3.05+-0.23 | 0.5+-0.23 | 4.55 |
Al I | ... | -4.36+-0.22 | -0.81+-0.22 | 2.09 |
Si I | ... | -3.20+-0.36 | 0.35+-0.36 | 4.31 |
Ca I | ... | -2.95+-0.23 | 0.6+-0.23 | 3.39 |
Sc II | ... | -3.74+-0.15 | -0.19+-0.15 | -0.14 |
Ti II | ... | -3.42+-0.14 | 0.13+-0.14 | 1.98 |
V II | ... | <-2.16 | <1.39 | <1.84 |
Cr I | ... | -3.80+-0.2 | -0.25+-0.2 | 1.84 |
Mn I | ... | -4.17+-0.21 | -0.62+-0.21 | 1.27 |
Fe I | ... | -3.55+-0.23 | ... | 3.95 |
Fe II | ... | -3.1+-0.14 | ... | 4.4 |
Co I | ... | -3.29+-0.23 | 0.26+-0.23 | 1.7 |
Ni I | ... | -3.66+-0.26 | -0.11+-0.26 | 2.56 |
Zn I | ... | <-2.15 | <1.40 | <2.45 |
Sr II | ... | -3.77+-0.2 | -0.22+-0.2 | -0.45 |
Y II | ... | <-3.07 | <0.48 | <-0.83 |
Zr II | ... | <-2.37 | <1.18 | <0.23 |
Nb II | ... | <0.27 | <3.82 | <1.69 |
Mo I | ... | <-1.07 | <2.48 | <0.85 |
Tc I | ... | <1.22 | <4.77 | <1.22 |
Ba II | ... | -4.30+-0.14 | -0.75+-0.14 | -1.67 |
Ce II | ... | <-1.69 | <1.86 | <-0.11 |
Pr II | ... | <-0.99 | <2.56 | <-0.28 |
Nd II | ... | <-1.67 | <1.88 | <-0.17 |
Sm II | ... | <-1.15 | <2.40 | <-0.14 |
Eu II | ... | <-1.88 | <1.67 | <-1.37 |
Gd II | ... | <-0.91 | <2.64 | <0.21 |
Tb II | ... | <-0.05 | <3.50 | <-0.15 |
Dy II | ... | <-1.63 | <1.92 | <-0.49 |
Ho II | ... | <-0.96 | <2.59 | <-0.7 |
Er II | ... | <-1.21 | <2.34 | <-0.28 |
Tm II | ... | <-0.45 | <3.10 | <-0.45 |
Yb II | ... | <-2.25 | <1.30 | <-1.17 |
Hf II | ... | <-0.10 | <3.45 | <0.78 |
Pb I | ... | <-0.41 | <3.14 | <1.54 |
Th II | ... | <-0.56 | <2.99 | <-0.56 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)