Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.66-0.2 | +-0.2 | 2.12 |
CH | ... | -2.57+-0.25 | 0.09+-0.25 | 6.08 |
CN | ... | <0.23 | <2.89 | <8.2 |
O I | ... | -2.29+-0.21 | 0.37+-0.21 | 6.39 |
Mg I | ... | -2.31+-0.22 | 0.35+-0.22 | 5.29 |
Al I | ... | -3.40+-0.28 | -0.74+-0.28 | 3.04 |
Si I | ... | -2.31+-0.36 | 0.35+-0.36 | 5.2 |
Ca I | ... | -2.17+-0.22 | 0.49+-0.22 | 4.17 |
Sc II | ... | -2.71+-0.15 | -0.05+-0.15 | 0.66 |
Ti I | ... | -2.22+-0.21 | 0.44+-0.21 | 2.73 |
Ti II | ... | -2.39+-0.14 | 0.27+-0.14 | 2.77 |
V II | ... | <-2.23 | <0.43 | <1.77 |
Cr I | ... | -2.71+-0.21 | -0.05+-0.21 | 2.93 |
Cr II | ... | -2.47+-0.15 | 0.19+-0.15 | 3.39 |
Mn I | ... | -2.92+-0.2 | -0.26+-0.2 | 2.51 |
Mn II | ... | -3.06+-0.23 | -0.4+-0.23 | 2.59 |
Fe I | ... | -2.66+-0.21 | ... | 4.84 |
Fe II | ... | -2.44+-0.15 | ... | 5.06 |
Co I | ... | -2.55+-0.23 | 0.11+-0.23 | 2.44 |
Ni I | ... | -2.64+-0.26 | 0.02+-0.26 | 3.58 |
Zn I | ... | <-2.09 | <0.57 | <2.51 |
Rb I | ... | <0.57 | <3.23 | <3.17 |
Sr II | ... | -2.66+-0.24 | 0.00+-0.24 | 0.43 |
Y II | ... | -2.88+-0.19 | -0.22+-0.19 | -0.45 |
Zr II | ... | -2.22+-0.17 | 0.44+-0.17 | 0.58 |
Nb II | ... | <0.08 | <2.74 | <1.5 |
Mo I | ... | <-0.57 | <2.09 | <1.35 |
Tc I | ... | <1.61 | <4.27 | <1.61 |
Ba II | ... | -3.05+-0.14 | -0.39+-0.14 | -0.65 |
Ce II | ... | <-1.29 | <1.37 | <0.29 |
Pr II | ... | <-0.81 | <1.85 | <-0.1 |
Nd II | ... | <-1.35 | <1.31 | <0.15 |
Sm II | ... | <-0.94 | <1.72 | <0.07 |
Eu II | ... | <-1.60 | <1.06 | <-1.09 |
Gd II | ... | <-0.67 | <1.99 | <0.45 |
Tb II | ... | <0.08 | <2.74 | <-0.02 |
Dy II | ... | <-1.32 | <1.34 | <-0.18 |
Ho II | ... | <-0.64 | <2.02 | <-0.38 |
Er II | ... | <-0.94 | <1.72 | <-0.01 |
Tm II | ... | <-0.37 | <2.29 | <-0.37 |
Yb II | ... | <-2.04 | <0.62 | <-0.96 |
Hf II | ... | <-0.11 | <2.55 | <0.77 |
Pb I | ... | <-0.09 | <2.57 | <1.86 |
Th II | ... | <-0.12 | <2.54 | <-0.12 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)