Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.84-0.2 | +-0.2 | 2 |
CH | ... | -2.82+-0.25 | 0.02+-0.25 | 5.87 |
NH | ... | <-1.67 | <1.17 | <6.3 |
O I | ... | -2.20+-0.2 | 0.64+-0.2 | 6.49 |
Mg I | ... | -2.57+-0.22 | 0.27+-0.22 | 5.03 |
Al I | ... | -3.66+-0.25 | -0.82+-0.25 | 2.79 |
Si I | ... | -2.52+-0.36 | 0.32+-0.36 | 4.99 |
K I | ... | -2.44+-0.25 | 0.4+-0.25 | 2.59 |
Ca I | ... | -2.38+-0.22 | 0.46+-0.22 | 3.96 |
Sc II | ... | -2.87+-0.16 | -0.03+-0.16 | 0.54 |
Ti I | ... | -2.50+-0.21 | 0.34+-0.21 | 2.45 |
Ti II | ... | -2.60+-0.15 | 0.24+-0.15 | 2.61 |
V II | ... | <-2.32 | <0.52 | <1.68 |
Cr I | ... | -2.99+-0.21 | -0.15+-0.21 | 2.65 |
Cr II | ... | -2.57+-0.16 | 0.27+-0.16 | 3.33 |
Mn I | ... | -3.12+-0.21 | -0.28+-0.21 | 2.31 |
Mn II | ... | -3.15+-0.21 | -0.31+-0.21 | 2.54 |
Fe I | ... | -2.84+-0.21 | ... | 4.66 |
Fe II | ... | -2.58+-0.15 | ... | 4.92 |
Co I | ... | -2.79+-0.24 | 0.05+-0.24 | 2.2 |
Ni I | ... | -2.87+-0.26 | -0.03+-0.26 | 3.35 |
Zn I | ... | <-2.27 | <0.57 | <2.33 |
Rb I | ... | <0.22 | <3.06 | <2.82 |
Sr II | ... | -3.27+-0.18 | -0.43+-0.18 | -0.14 |
Y II | ... | -3.50+-0.25 | -0.66+-0.25 | -1.03 |
Zr II | ... | -2.79+-0.21 | 0.05+-0.21 | 0.05 |
Nb II | ... | <-0.21 | <2.63 | <1.21 |
Mo I | ... | <-0.84 | <2.00 | <1.08 |
Tc I | ... | <1.33 | <4.17 | <1.33 |
Ba II | ... | -4.35+-0.21 | -1.51+-0.21 | -1.91 |
La II | ... | <-1.98 | <0.86 | <-0.81 |
Ce II | ... | <-1.62 | <1.22 | <-0.04 |
Pr II | ... | <-1.13 | <1.71 | <-0.42 |
Nd II | ... | <-1.85 | <0.99 | <-0.35 |
Sm II | ... | <-1.17 | <1.67 | <-0.16 |
Eu II | ... | <-1.97 | <0.87 | <-1.46 |
Gd II | ... | <-1.01 | <1.83 | <0.11 |
Tb II | ... | <-0.25 | <2.59 | <-0.35 |
Dy II | ... | <-1.60 | <1.24 | <-0.46 |
Ho II | ... | <-0.69 | <2.15 | <-0.43 |
Er II | ... | <-1.14 | <1.70 | <-0.21 |
Tm II | ... | <-0.73 | <2.11 | <-0.73 |
Yb II | ... | <-2.57 | <0.27 | <-1.49 |
Hf II | ... | <-0.35 | <2.49 | <0.53 |
Pb I | ... | <-0.58 | <2.26 | <1.37 |
Th II | ... | <-0.46 | <2.38 | <-0.46 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)