Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.29 | <2.81 | <1.45 |
CH | ... | <-1.75 | <0.77 | <6.8 |
NH | ... | <-0.37 | <2.15 | <7.6 |
O I | ... | -2.23+-0.16 | 0.29+-0.16 | 6.46 |
Mg I | ... | -2.10+-0.17 | 0.42+-0.17 | 5.5 |
Al I | ... | -3.11+-0.23 | -0.59+-0.23 | 3.34 |
Si I | ... | -2.43+-0.31 | 0.09+-0.31 | 5.08 |
Ca I | ... | -2.07+-0.19 | 0.45+-0.19 | 4.27 |
Sc II | ... | -2.37+-0.15 | 0.15+-0.15 | 0.79 |
Ti I | ... | -2.03+-0.17 | 0.49+-0.17 | 2.92 |
Ti II | ... | -2.20+-0.15 | 0.32+-0.15 | 2.76 |
V II | ... | -2.26+-0.24 | 0.26+-0.24 | 1.68 |
Cr I | ... | -2.45+-0.17 | 0.07+-0.17 | 3.19 |
Cr II | ... | -2.34+-0.16 | 0.18+-0.16 | 3.3 |
Mn I | ... | -2.74+-0.17 | -0.22+-0.17 | 2.68 |
Fe I | ... | -2.52+-0.17 | ... | 4.98 |
Fe II | ... | -2.51+-0.15 | ... | 4.99 |
Co I | ... | -2.41+-0.2 | 0.11+-0.2 | 2.58 |
Ni I | ... | -2.45+-0.19 | 0.07+-0.19 | 3.77 |
Zn I | ... | -2.24+-0.19 | 0.28+-0.19 | 2.32 |
Rb I | ... | <-0.03 | <2.49 | <2.57 |
Sr II | ... | -2.36+-0.25 | 0.16+-0.25 | 0.51 |
Y II | ... | -2.84+-0.18 | -0.32+-0.18 | -0.63 |
Zr II | ... | -2.19+-0.16 | 0.33+-0.16 | 0.4 |
Nb II | ... | <-0.43 | <2.09 | <0.99 |
Mo I | ... | <-0.69 | <1.83 | <1.23 |
Tc I | ... | <1.27 | <3.79 | <1.27 |
Ba II | ... | -2.76+-0.15 | -0.24+-0.15 | -0.58 |
La II | ... | <-2.28 | <0.24 | <-1.11 |
Ce II | ... | <-2.30 | <0.22 | <-0.72 |
Pr II | ... | <-1.77 | <0.75 | <-1.06 |
Nd II | ... | <-2.19 | <0.33 | <-0.69 |
Sm II | ... | <-1.83 | <0.69 | <-0.82 |
Eu II | ... | -2.05+-0.17 | 0.47+-0.17 | -1.53 |
Gd II | ... | <-1.49 | <1.03 | <-0.37 |
Tb II | ... | <-0.66 | <1.86 | <-0.76 |
Dy II | ... | -2.11+-0.19 | 0.41+-0.19 | -1 |
Er II | ... | <-1.56 | <0.96 | <-0.63 |
Tm II | ... | <-1.14 | <1.38 | <-1.14 |
Yb II | ... | -2.61+-0.26 | -0.09+-0.26 | -1.68 |
Hf II | ... | <-0.93 | <1.59 | <-0.05 |
Pb I | ... | <-0.35 | <2.17 | <1.6 |
Th II | ... | <-0.99 | <1.53 | <-0.99 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)