Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.63-0.2 | +-0.2 | 2.06 |
CH | ... | -2.37+-0.25 | 0.26+-0.25 | 6.18 |
NH | ... | <-1.72 | <0.91 | <6.25 |
O I | ... | -2.35+-0.21 | 0.28+-0.21 | 6.34 |
Mg I | ... | -2.38+-0.22 | 0.25+-0.22 | 5.21 |
Al I | ... | -3.51+-0.26 | -0.88+-0.26 | 2.94 |
Si I | ... | -2.25+-0.36 | 0.38+-0.36 | 5.26 |
Ca I | ... | -2.23+-0.22 | 0.4+-0.22 | 4.11 |
Sc II | ... | -2.86+-0.17 | -0.23+-0.17 | 0.41 |
Ti I | ... | -2.32+-0.21 | 0.31+-0.21 | 2.63 |
Ti II | ... | -2.50+-0.15 | 0.13+-0.15 | 2.57 |
V II | ... | <-2.24 | <0.39 | <1.76 |
Cr I | ... | -2.76+-0.21 | -0.13+-0.21 | 2.88 |
Cr II | ... | -2.59+-0.18 | 0.04+-0.18 | 3.17 |
Mn I | ... | -3.02+-0.2 | -0.39+-0.2 | 2.41 |
Mn II | ... | -3.06+-0.2 | -0.43+-0.2 | 2.5 |
Fe I | ... | -2.63+-0.21 | ... | 4.87 |
Fe II | ... | -2.51+-0.15 | ... | 4.99 |
Co I | ... | -2.61+-0.24 | 0.02+-0.24 | 2.38 |
Ni I | ... | -2.75+-0.26 | -0.12+-0.26 | 3.47 |
Zn I | ... | <-2.13 | <0.50 | <2.47 |
Sr II | ... | -2.70+-0.23 | -0.07+-0.23 | 0.29 |
Y II | ... | -3.03+-0.32 | -0.4+-0.32 | -0.7 |
Zr II | ... | -2.45+-0.2 | 0.18+-0.2 | 0.25 |
Nb II | ... | <0.08 | <2.71 | <1.5 |
Mo I | ... | <-0.88 | <1.75 | <1.04 |
Tc I | ... | <1.43 | <4.06 | <1.43 |
Ba II | ... | -3.09+-0.14 | -0.46+-0.14 | -0.79 |
Ce II | ... | <-1.41 | <1.22 | <0.17 |
Pr II | ... | <-1.00 | <1.63 | <-0.29 |
Nd II | ... | <-1.45 | <1.18 | <0.05 |
Sm II | ... | <-0.98 | <1.65 | <0.03 |
Eu II | ... | <-1.68 | <0.95 | <-1.17 |
Gd II | ... | <-0.79 | <1.84 | <0.33 |
Tb II | ... | <-0.07 | <2.56 | <-0.17 |
Dy II | ... | <-1.30 | <1.33 | <-0.16 |
Ho II | ... | <-0.67 | <1.96 | <-0.41 |
Er II | ... | <-1.02 | <1.61 | <-0.09 |
Tm II | ... | <-0.36 | <2.27 | <-0.36 |
Yb II | ... | <-2.16 | <0.47 | <-1.08 |
Hf II | ... | <-0.30 | <2.33 | <0.58 |
Pb I | ... | <-0.23 | <2.40 | <1.72 |
Th II | ... | <-0.24 | <2.39 | <-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)