Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.81-0.2 | +-0.2 | 2.06 |
CH | ... | -2.60+-0.25 | 0.21+-0.25 | 6.16 |
CN | ... | <-0.42 | <2.39 | <7.55 |
O I | ... | -2.16+-0.21 | 0.65+-0.21 | 6.53 |
Mg I | ... | -2.40+-0.22 | 0.41+-0.22 | 5.2 |
Al I | ... | -3.53+-0.28 | -0.72+-0.28 | 2.93 |
Si I | ... | -2.39+-0.36 | 0.42+-0.36 | 5.12 |
Ca I | ... | -2.21+-0.22 | 0.6+-0.22 | 4.13 |
Sc II | ... | -2.91+-0.15 | -0.1+-0.15 | 0.57 |
Ti I | ... | -2.34+-0.2 | 0.47+-0.2 | 2.61 |
Ti II | ... | -2.51+-0.14 | 0.3+-0.14 | 2.77 |
V II | ... | <-2.20 | <0.61 | <1.8 |
Cr I | ... | -3.01+-0.2 | -0.2+-0.2 | 2.63 |
Cr II | ... | -2.48+-0.16 | 0.33+-0.16 | 3.49 |
Mn I | ... | -3.35+-0.2 | -0.54+-0.2 | 2.08 |
Fe I | ... | -2.81+-0.21 | ... | 4.69 |
Fe II | ... | -2.48+-0.14 | ... | 5.02 |
Co I | ... | -2.70+-0.23 | 0.11+-0.23 | 2.29 |
Ni I | ... | -2.78+-0.24 | 0.03+-0.24 | 3.44 |
Zn I | ... | -2.19+-0.22 | 0.62+-0.22 | 2.37 |
Rb I | ... | <0.38 | <3.19 | <2.98 |
Sr II | ... | -2.78+-0.24 | 0.03+-0.24 | 0.42 |
Y II | ... | -3.17+-0.2 | -0.36+-0.2 | -0.63 |
Zr II | ... | -2.56+-0.17 | 0.25+-0.17 | 0.35 |
Nb II | ... | <0.20 | <3.01 | <1.62 |
Mo I | ... | <-0.71 | <2.10 | <1.21 |
Tc I | ... | <1.48 | <4.29 | <1.48 |
Sn I | ... | <0.49 | <3.30 | <2.49 |
Ba II | ... | -3.20+-0.14 | -0.39+-0.14 | -0.69 |
Ce II | ... | <-1.55 | <1.26 | <0.03 |
Pr II | ... | <-0.89 | <1.92 | <-0.18 |
Nd II | ... | <-1.54 | <1.27 | <-0.04 |
Sm II | ... | <-0.91 | <1.90 | <0.1 |
Eu II | ... | <-1.70 | <1.11 | <-1.19 |
Gd II | ... | <-0.81 | <2.00 | <0.31 |
Tb II | ... | <-0.16 | <2.65 | <-0.26 |
Er II | ... | <-1.10 | <1.71 | <-0.17 |
Tm II | ... | <-0.52 | <2.29 | <-0.52 |
Yb II | ... | <-2.13 | <0.68 | <-1.05 |
Hf II | ... | <-0.26 | <2.55 | <0.62 |
Pb I | ... | <-0.38 | <2.43 | <1.57 |
Th II | ... | <-0.11 | <2.70 | <-0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)