Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.80 | <3.38 | <1.96 |
CH | ... | <-1.15 | <1.43 | <7.4 |
CN | ... | <-0.47 | <2.11 | <7.5 |
O I | ... | -2.55+-0.17 | 0.03+-0.17 | 6.14 |
Mg I | ... | -2.12+-0.17 | 0.46+-0.17 | 5.48 |
Al I | ... | -3.16+-0.21 | -0.58+-0.21 | 3.29 |
Si I | ... | -2.26+-0.31 | 0.32+-0.31 | 5.25 |
Ca I | ... | -2.19+-0.19 | 0.39+-0.19 | 4.15 |
Sc II | ... | -2.33+-0.16 | 0.25+-0.16 | 0.8 |
Ti I | ... | -2.07+-0.17 | 0.51+-0.17 | 2.88 |
Ti II | ... | -2.18+-0.15 | 0.4+-0.15 | 2.74 |
V II | ... | -2.13+-0.24 | 0.45+-0.24 | 1.78 |
Cr I | ... | -2.64+-0.17 | -0.06+-0.17 | 3 |
Cr II | ... | -2.38+-0.15 | 0.2+-0.15 | 3.24 |
Mn I | ... | -2.68+-0.17 | -0.1+-0.17 | 2.75 |
Mn II | ... | -2.76+-0.21 | -0.18+-0.21 | 2.65 |
Fe I | ... | -2.58+-0.17 | ... | 4.92 |
Fe II | ... | -2.6+-0.15 | ... | 4.9 |
Co I | ... | -2.31+-0.2 | 0.27+-0.2 | 2.68 |
Ni I | ... | -2.28+-0.21 | 0.3+-0.21 | 3.94 |
Zn I | ... | <-1.78 | <0.80 | <2.82 |
Rb I | ... | <0.64 | <3.22 | <3.24 |
Sr II | ... | -2.61+-0.25 | -0.03+-0.25 | 0.23 |
Y II | ... | -2.84+-0.2 | -0.26+-0.2 | -0.65 |
Zr II | ... | -2.25+-0.17 | 0.33+-0.17 | 0.31 |
Nb II | ... | <-0.10 | <2.48 | <1.32 |
Mo I | ... | <-0.30 | <2.28 | <1.62 |
Tc I | ... | <1.93 | <4.51 | <1.93 |
Ba II | ... | -2.97+-0.15 | -0.39+-0.15 | -0.82 |
Ce II | ... | <-1.73 | <0.85 | <-0.15 |
Pr II | ... | <-1.29 | <1.29 | <-0.58 |
Nd II | ... | <-1.81 | <0.77 | <-0.31 |
Sm II | ... | <-1.27 | <1.31 | <-0.26 |
Eu II | ... | <-1.68 | <0.90 | <-1.17 |
Gd II | ... | <-1.08 | <1.50 | <0.04 |
Tb II | ... | <-0.37 | <2.21 | <-0.47 |
Dy II | ... | <-1.55 | <1.03 | <-0.41 |
Ho II | ... | <-0.88 | <1.70 | <-0.62 |
Er II | ... | <-1.40 | <1.18 | <-0.47 |
Tm II | ... | <-0.84 | <1.74 | <-0.84 |
Yb II | ... | <-2.47 | <0.11 | <-1.39 |
Hf II | ... | <-0.48 | <2.10 | <0.4 |
Pb I | ... | <0.01 | <2.59 | <1.96 |
Th II | ... | <-0.43 | <2.15 | <-0.43 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)