Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.82-0.2 | +-0.2 | 2.11 |
CH | ... | -2.55+-0.25 | 0.27+-0.25 | 5.99 |
NH | ... | <-1.92 | <0.90 | <6.05 |
O I | ... | -1.94+-0.21 | 0.88+-0.21 | 6.75 |
Mg I | ... | -2.38+-0.22 | 0.44+-0.22 | 5.22 |
Al I | ... | -3.52+-0.28 | -0.7+-0.28 | 2.93 |
Si I | ... | -2.22+-0.36 | 0.6+-0.36 | 5.29 |
Ca I | ... | -2.34+-0.22 | 0.48+-0.22 | 4 |
Sc II | ... | -2.86+-0.15 | -0.04+-0.15 | 0.39 |
Ti I | ... | -2.45+-0.21 | 0.37+-0.21 | 2.5 |
Ti II | ... | -2.60+-0.15 | 0.22+-0.15 | 2.46 |
V II | ... | <-2.44 | <0.38 | <1.56 |
Cr I | ... | -3.06+-0.21 | -0.24+-0.21 | 2.58 |
Cr II | ... | -2.64+-0.18 | 0.18+-0.18 | 3.1 |
Mn I | ... | -3.24+-0.22 | -0.42+-0.22 | 2.19 |
Mn II | ... | -3.22+-0.21 | -0.4+-0.21 | 2.32 |
Fe I | ... | -2.82+-0.21 | ... | 4.68 |
Fe II | ... | -2.72+-0.15 | ... | 4.78 |
Co I | ... | -2.69+-0.24 | 0.13+-0.24 | 2.3 |
Ni I | ... | -2.83+-0.27 | -0.01+-0.27 | 3.39 |
Zn I | ... | <-2.11 | <0.71 | <2.49 |
Rb I | ... | <0.07 | <2.89 | <2.67 |
Sr II | ... | -2.95+-0.19 | -0.13+-0.19 | 0.02 |
Y II | ... | -3.41+-0.32 | -0.59+-0.32 | -1.1 |
Nb II | ... | <-0.19 | <2.63 | <1.23 |
Mo I | ... | <-0.88 | <1.94 | <1.04 |
Tc I | ... | <1.23 | <4.05 | <1.23 |
Ba II | ... | -3.48+-0.14 | -0.66+-0.14 | -1.2 |
Ce II | ... | <-1.73 | <1.09 | <-0.15 |
Pr II | ... | <-1.35 | <1.47 | <-0.64 |
Nd II | ... | <-1.22 | <1.60 | <0.28 |
Sm II | ... | <-1.12 | <1.70 | <-0.11 |
Eu II | ... | <-2.04 | <0.78 | <-1.53 |
Gd II | ... | <-1.06 | <1.76 | <0.06 |
Tb II | ... | <-0.19 | <2.63 | <-0.29 |
Dy II | ... | <-1.49 | <1.33 | <-0.35 |
Ho II | ... | <-1.12 | <1.70 | <-0.86 |
Er II | ... | <-1.47 | <1.35 | <-0.54 |
Tm II | ... | <-0.81 | <2.01 | <-0.81 |
Yb II | ... | <-2.35 | <0.47 | <-1.27 |
Hf II | ... | <-0.61 | <2.21 | <0.27 |
Pb I | ... | <-0.45 | <2.37 | <1.5 |
Th II | ... | <-0.58 | <2.24 | <-0.58 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)