Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <1.65 | <4.03 | <2.81 |
CH | ... | <0.50 | <2.88 | <9.05 |
CN | ... | <0.83 | <3.21 | <8.8 |
O I | ... | -1.96+-0.16 | 0.42+-0.16 | 6.73 |
Mg I | ... | -1.96+-0.17 | 0.42+-0.17 | 5.64 |
Al I | ... | -2.70+-0.18 | -0.32+-0.18 | 3.75 |
Si I | ... | -2.28+-0.23 | 0.1+-0.23 | 5.23 |
Ca I | ... | -2.04+-0.2 | 0.34+-0.2 | 4.3 |
Sc II | ... | -2.22+-0.15 | 0.16+-0.15 | 0.95 |
Ti II | ... | -2.08+-0.15 | 0.3+-0.15 | 2.89 |
V II | ... | <-1.94 | <0.44 | <2.06 |
Cr I | ... | -2.33+-0.17 | 0.05+-0.17 | 3.3 |
Cr II | ... | -2.17+-0.15 | 0.21+-0.15 | 3.5 |
Mn I | ... | <-1.69 | <0.69 | <3.7 |
Mn II | ... | <-1.81 | <0.57 | <3.58 |
Fe I | ... | -2.38+-0.17 | ... | 5.12 |
Fe II | ... | -2.35+-0.15 | ... | 5.15 |
Cu I | ... | <-0.28 | <2.10 | <3.93 |
Zn I | ... | <-1.09 | <1.29 | <3.51 |
Rb I | ... | <1.29 | <3.67 | <3.89 |
Sr II | ... | -2.80+-0.15 | -0.42+-0.15 | 0.1 |
Y II | ... | <-2.14 | <0.24 | <0.1 |
Zr II | ... | <-1.73 | <0.65 | <0.87 |
Nb II | ... | <0.42 | <2.80 | <1.84 |
Mo I | ... | <0.91 | <3.29 | <2.83 |
Tc I | ... | <3.12 | <5.50 | <3.12 |
Ba II | ... | -2.67+-0.16 | -0.29+-0.16 | -0.46 |
Ce II | ... | <-0.79 | <1.59 | <0.79 |
Pr II | ... | <-0.07 | <2.31 | <0.64 |
Nd II | ... | <-0.57 | <1.81 | <0.93 |
Sm II | ... | <-0.21 | <2.17 | <0.8 |
Eu II | ... | <-0.93 | <1.45 | <-0.42 |
Gd II | ... | <-0.23 | <2.15 | <0.89 |
Tb II | ... | <0.73 | <3.11 | <0.63 |
Dy II | ... | <-0.54 | <1.84 | <0.6 |
Ho II | ... | <0.01 | <2.39 | <0.27 |
Er II | ... | <-0.20 | <2.18 | <0.73 |
Tm II | ... | <0.18 | <2.56 | <0.18 |
Yb II | ... | <-1.19 | <1.19 | <-0.11 |
Hf II | ... | <0.34 | <2.72 | <1.22 |
Pb I | ... | <1.06 | <3.44 | <3.01 |
Th II | ... | <0.53 | <2.91 | <0.53 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)