Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.10-0.2 | +-0.2 | 1.96 |
CH | ... | -2.63+-0.25 | 0.47+-0.25 | 5.79 |
CN | ... | <-0.47 | <2.63 | <7.5 |
O I | ... | <-2.43 | <0.67 | <6.44 |
Mg I | ... | -2.72+-0.22 | 0.38+-0.22 | 4.88 |
Al I | ... | -3.82+-0.25 | -0.72+-0.25 | 2.63 |
Si I | ... | -2.41+-0.36 | 0.69+-0.36 | 5.1 |
Ca I | ... | -2.69+-0.23 | 0.41+-0.23 | 3.64 |
Sc II | ... | -3.28+-0.14 | -0.18+-0.14 | -0.14 |
Ti I | ... | -2.61+-0.21 | 0.49+-0.21 | 2.33 |
Ti II | ... | -3.02+-0.13 | 0.08+-0.13 | 1.92 |
V II | ... | <-2.28 | <0.82 | <1.72 |
Cr I | ... | -3.29+-0.2 | -0.19+-0.2 | 2.35 |
Mn I | ... | -3.60+-0.2 | -0.5+-0.2 | 1.83 |
Fe I | ... | -3.1+-0.21 | ... | 4.4 |
Fe II | ... | -3.11+-0.15 | ... | 4.39 |
Co I | ... | -3.06+-0.24 | 0.04+-0.24 | 1.93 |
Ni I | ... | -3.07+-0.25 | 0.03+-0.25 | 3.15 |
Zn I | ... | <-2.21 | <0.89 | <2.39 |
Ga I | ... | <-1.38 | <1.72 | <1.5 |
Rb I | ... | <0.02 | <3.12 | <2.62 |
Sr II | ... | -3.29+-0.18 | -0.19+-0.18 | -0.43 |
Y II | ... | <-3.04 | <0.06 | <-0.8 |
Zr II | ... | <-2.27 | <0.83 | <0.33 |
Nb II | ... | <0.09 | <3.19 | <1.51 |
Mo I | ... | <-0.92 | <2.18 | <1 |
Tc I | ... | <1.36 | <4.46 | <1.36 |
Ba II | ... | -3.68+-0.14 | -0.58+-0.14 | -1.51 |
Ce II | ... | <-1.78 | <1.32 | <-0.2 |
Pr II | ... | <-1.10 | <2.00 | <-0.39 |
Nd II | ... | <-1.56 | <1.54 | <-0.06 |
Sm II | ... | <-1.09 | <2.01 | <-0.08 |
Eu II | ... | <-1.91 | <1.19 | <-1.4 |
Gd II | ... | <-0.82 | <2.28 | <0.3 |
Tb II | ... | <-0.32 | <2.78 | <-0.42 |
Dy II | ... | <-1.57 | <1.53 | <-0.43 |
Ho II | ... | <-0.91 | <2.19 | <-0.65 |
Er II | ... | <-1.12 | <1.98 | <-0.19 |
Tm II | ... | <-0.75 | <2.35 | <-0.75 |
Yb II | ... | <-2.02 | <1.08 | <-0.94 |
Hf II | ... | <-0.31 | <2.79 | <0.57 |
Pb I | ... | <-0.05 | <3.05 | <1.9 |
Th II | ... | <-0.45 | <2.65 | <-0.45 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)