Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.98-0.2 | +-0.2 | 1.97 |
CH | ... | -2.60+-0.25 | 0.38+-0.25 | 5.77 |
NH | ... | <-2.02 | <0.96 | <5.95 |
Mg I | ... | -2.57+-0.22 | 0.41+-0.22 | 5.03 |
Al I | ... | -3.70+-0.25 | -0.72+-0.25 | 2.76 |
Si I | ... | -2.24+-0.36 | 0.74+-0.36 | 5.27 |
Ca I | ... | -2.55+-0.22 | 0.43+-0.22 | 3.79 |
Sc II | ... | -2.90+-0.16 | 0.08+-0.16 | 0.19 |
Ti I | ... | -2.64+-0.21 | 0.34+-0.21 | 2.32 |
Ti II | ... | -2.80+-0.15 | 0.18+-0.15 | 2.09 |
V II | ... | <-2.45 | <0.53 | <1.55 |
Cr I | ... | -3.27+-0.2 | -0.29+-0.2 | 2.38 |
Mn I | ... | -3.51+-0.21 | -0.53+-0.21 | 1.92 |
Mn II | ... | -3.47+-0.21 | -0.49+-0.21 | 1.9 |
Fe I | ... | -2.98+-0.22 | ... | 4.52 |
Fe II | ... | -3.04+-0.16 | ... | 4.46 |
Co I | ... | -2.91+-0.24 | 0.07+-0.24 | 2.08 |
Ni I | ... | -3.03+-0.26 | -0.05+-0.26 | 3.19 |
Zn I | ... | <-1.47 | <1.51 | <3.13 |
Sr II | ... | -3.23+-0.15 | -0.25+-0.15 | -0.42 |
Y II | ... | <-3.36 | <-0.38 | <-1.12 |
Zr II | ... | <-2.34 | <0.64 | <0.26 |
Nb II | ... | <-0.02 | <2.96 | <1.4 |
Mo I | ... | <-0.75 | <2.23 | <1.17 |
Tc I | ... | <1.25 | <4.23 | <1.25 |
Ba II | ... | -3.57+-0.14 | -0.59+-0.14 | -1.45 |
Ce II | ... | <-1.67 | <1.31 | <-0.09 |
Pr II | ... | <-1.24 | <1.74 | <-0.53 |
Nd II | ... | <-1.51 | <1.47 | <-0.01 |
Sm II | ... | <-1.24 | <1.74 | <-0.23 |
Eu II | ... | <-1.86 | <1.12 | <-1.35 |
Gd II | ... | <-1.02 | <1.96 | <0.1 |
Tb II | ... | <-0.29 | <2.69 | <-0.39 |
Dy II | ... | <-1.63 | <1.35 | <-0.49 |
Ho II | ... | <-0.96 | <2.02 | <-0.7 |
Er II | ... | <-1.27 | <1.71 | <-0.34 |
Tm II | ... | <-0.74 | <2.24 | <-0.74 |
Yb II | ... | <-2.33 | <0.65 | <-1.25 |
Hf II | ... | <-0.35 | <2.63 | <0.53 |
Pb I | ... | <-0.61 | <2.37 | <1.34 |
Th II | ... | <-0.42 | <2.56 | <-0.42 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)