Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.54 | <3.30 | <1.7 |
CH | ... | -1.67+-0.25 | 1.09+-0.25 | 6.78 |
NH | ... | -0.47+-0.36 | 2.29+-0.36 | 7.38 |
O I | ... | -2.63+-0.22 | 0.13+-0.22 | 6.06 |
Na I | ... | -2.27+-0.31 | 0.49+-0.31 | 3.97 |
Mg I | ... | -2.39+-0.21 | 0.37+-0.21 | 5.21 |
Al I | ... | -3.40+-0.26 | -0.64+-0.26 | 3.05 |
Si I | ... | -2.29+-0.36 | 0.47+-0.36 | 5.22 |
Ca I | ... | -2.28+-0.22 | 0.48+-0.22 | 4.06 |
Sc II | ... | -2.68+-0.15 | 0.08+-0.15 | 0.48 |
Ti I | ... | -2.38+-0.22 | 0.38+-0.22 | 2.57 |
Ti II | ... | -2.40+-0.14 | 0.36+-0.14 | 2.56 |
V II | ... | <-2.18 | <0.58 | <1.82 |
Cr I | ... | -2.91+-0.2 | -0.15+-0.2 | 2.73 |
Cr II | ... | -2.34+-0.18 | 0.42+-0.18 | 3.31 |
Mn I | ... | -3.18+-0.21 | -0.42+-0.21 | 2.26 |
Fe I | ... | -2.76+-0.21 | ... | 4.74 |
Fe II | ... | -2.75+-0.15 | ... | 4.75 |
Co I | ... | -2.52+-0.24 | 0.24+-0.24 | 2.47 |
Ni I | ... | -2.76+-0.25 | 0.00+-0.25 | 3.46 |
Zn I | ... | <-2.02 | <0.74 | <2.58 |
Rb I | ... | <0.21 | <2.97 | <2.81 |
Sr II | ... | -2.20+-0.24 | 0.56+-0.24 | 0.68 |
Zr II | ... | -2.00+-0.18 | 0.76+-0.18 | 0.59 |
Nb II | ... | <0.30 | <3.06 | <1.72 |
Mo I | ... | <-0.45 | <2.31 | <1.47 |
Ba II | ... | -2.15+-0.14 | 0.61+-0.14 | 0.04 |
La II | ... | <-1.59 | <1.17 | <-0.42 |
Ce II | ... | <-1.29 | <1.47 | <0.29 |
Pr II | ... | <-0.79 | <1.97 | <-0.08 |
Nd II | ... | <-0.91 | <1.85 | <0.59 |
Sm II | ... | <-0.87 | <1.89 | <0.14 |
Eu II | ... | <-1.51 | <1.25 | <-1 |
Gd II | ... | <-0.57 | <2.19 | <0.55 |
Tb II | ... | <0.07 | <2.83 | <-0.03 |
Dy II | ... | <-1.11 | <1.65 | <0.03 |
Ho II | ... | <-0.40 | <2.36 | <-0.14 |
Er II | ... | <-0.64 | <2.12 | <0.29 |
Tm II | ... | <-0.22 | <2.54 | <-0.22 |
Yb II | ... | <-1.75 | <1.01 | <-0.67 |
Hf II | ... | <-0.05 | <2.71 | <0.83 |
Pb I | ... | <-0.05 | <2.71 | <1.9 |
Th II | ... | <0.04 | <2.80 | <0.04 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)