Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.82-0.2 | +-0.2 | 1.9 |
CH | ... | -2.46+-0.25 | 0.36+-0.25 | 6.09 |
NH | ... | <-1.62 | <1.20 | <6.35 |
O I | ... | -2.38+-0.21 | 0.44+-0.21 | 6.31 |
Mg I | ... | -2.40+-0.22 | 0.42+-0.22 | 5.2 |
Al I | ... | -3.53+-0.26 | -0.71+-0.26 | 2.92 |
Si I | ... | -2.44+-0.36 | 0.38+-0.36 | 5.07 |
Ca I | ... | -2.24+-0.22 | 0.58+-0.22 | 4.1 |
Sc II | ... | -2.80+-0.15 | 0.02+-0.15 | 0.47 |
Ti I | ... | -2.46+-0.21 | 0.36+-0.21 | 2.49 |
Ti II | ... | -2.52+-0.14 | 0.3+-0.14 | 2.55 |
V I | ... | <-2.10 | <0.72 | <1.9 |
V II | ... | <-1.97 | <0.85 | <2.03 |
Cr I | ... | -3.06+-0.2 | -0.24+-0.2 | 2.58 |
Mn I | ... | -3.20+-0.2 | -0.38+-0.2 | 2.23 |
Mn II | ... | -2.99+-0.22 | -0.17+-0.22 | 2.56 |
Fe I | ... | -2.82+-0.21 | ... | 4.68 |
Fe II | ... | -2.7+-0.14 | ... | 4.8 |
Co I | ... | -2.78+-0.24 | 0.04+-0.24 | 2.21 |
Ni I | ... | -2.90+-0.28 | -0.08+-0.28 | 3.32 |
Zn I | ... | -2.39+-0.24 | 0.43+-0.24 | 2.17 |
Rb I | ... | <0.25 | <3.07 | <2.85 |
Sr II | ... | -2.32+-0.24 | 0.5+-0.24 | 0.68 |
Y II | ... | -2.61+-0.21 | 0.21+-0.21 | -0.28 |
Zr II | ... | -2.11+-0.16 | 0.71+-0.16 | 0.59 |
Nb II | ... | <0.21 | <3.03 | <1.63 |
Mo I | ... | <-0.58 | <2.24 | <1.34 |
Tc I | ... | <1.58 | <4.40 | <1.58 |
Ba II | ... | -3.21+-0.14 | -0.39+-0.14 | -0.91 |
Ce II | ... | <-1.38 | <1.44 | <0.2 |
Pr II | ... | <-0.89 | <1.93 | <-0.18 |
Nd II | ... | <-1.45 | <1.37 | <0.05 |
Sm II | ... | <-0.98 | <1.84 | <0.03 |
Eu II | ... | <-1.65 | <1.17 | <-1.14 |
Gd II | ... | <-0.71 | <2.11 | <0.41 |
Tb II | ... | <0.03 | <2.85 | <-0.07 |
Dy II | ... | <-1.19 | <1.63 | <-0.05 |
Ho II | ... | <-0.42 | <2.40 | <-0.16 |
Er II | ... | <-0.86 | <1.96 | <0.07 |
Tm II | ... | <-0.31 | <2.51 | <-0.31 |
Yb II | ... | <-2.09 | <0.73 | <-1.01 |
Hf II | ... | <-0.01 | <2.81 | <0.87 |
Pb I | ... | <-0.29 | <2.53 | <1.66 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)