Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.30-0.2 | +-0.2 | 1.85 |
CH | ... | -2.55+-0.25 | 0.75+-0.25 | 5.78 |
NH | ... | <-1.87 | <1.43 | <6.1 |
O I | ... | <-2.39 | <0.91 | <6.48 |
Mg I | ... | -2.62+-0.23 | 0.68+-0.23 | 4.98 |
Al I | ... | -3.97+-0.26 | -0.67+-0.26 | 2.48 |
Si I | ... | -2.43+-0.36 | 0.87+-0.36 | 5.08 |
Ca I | ... | -2.69+-0.22 | 0.61+-0.22 | 3.65 |
Sc II | ... | -3.16+-0.15 | 0.14+-0.15 | -0.11 |
Ti I | ... | -3.03+-0.21 | 0.27+-0.21 | 1.92 |
Ti II | ... | -3.21+-0.14 | 0.09+-0.14 | 1.64 |
V II | ... | <-2.47 | <0.83 | <1.53 |
Cr I | ... | -3.66+-0.2 | -0.36+-0.2 | 1.98 |
Mn I | ... | -4.01+-0.21 | -0.71+-0.21 | 1.42 |
Fe I | ... | -3.3+-0.22 | ... | 4.2 |
Fe II | ... | -3.4+-0.16 | ... | 4.1 |
Co I | ... | -3.21+-0.25 | 0.09+-0.25 | 1.78 |
Ni I | ... | -3.39+-0.25 | -0.09+-0.25 | 2.83 |
Zn I | ... | <-2.49 | <0.81 | <2.11 |
Ga I | ... | <-1.73 | <1.57 | <1.15 |
Rb I | ... | <-0.25 | <3.05 | <2.35 |
Sr II | ... | <-5.20 | <-1.90 | <-2.23 |
Y II | ... | <-3.59 | <-0.29 | <-1.35 |
Zr II | ... | <-2.15 | <1.15 | <0.45 |
Mo I | ... | <-1.18 | <2.12 | <0.74 |
Tc I | ... | <1.02 | <4.32 | <1.02 |
Ba II | ... | <-3.31 | <-0.01 | <-1.18 |
La II | ... | <-2.10 | <1.20 | <-0.93 |
Ce II | ... | <-2.00 | <1.30 | <-0.42 |
Pr II | ... | <-1.51 | <1.79 | <-0.8 |
Nd II | ... | <-1.92 | <1.38 | <-0.42 |
Sm II | ... | <-1.44 | <1.86 | <-0.43 |
Eu II | ... | <-2.01 | <1.29 | <-1.5 |
Gd II | ... | <-1.27 | <2.03 | <-0.15 |
Tb II | ... | <-0.40 | <2.90 | <-0.5 |
Dy II | ... | <-1.76 | <1.54 | <-0.62 |
Ho II | ... | <-1.01 | <2.29 | <-0.75 |
Er II | ... | <-1.28 | <2.02 | <-0.35 |
Tm II | ... | <-0.96 | <2.34 | <-0.96 |
Yb II | ... | <-2.53 | <0.77 | <-1.45 |
Hf II | ... | <-0.57 | <2.73 | <0.31 |
Pb I | ... | <-0.45 | <2.85 | <1.5 |
Th II | ... | <-0.63 | <2.67 | <-0.63 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)