Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.61-0.15 | +-0.15 | 0.89 |
CH | ... | -3.34+-0.25 | 0.27+-0.25 | 5.17 |
NH | ... | -2.96+-0.36 | 0.65+-0.36 | 4.95 |
O I | ... | <-2.58 | <1.03 | <6.29 |
Mg I | ... | -3.05+-0.15 | 0.56+-0.15 | 4.55 |
Al I | ... | -4.36+-0.23 | -0.75+-0.23 | 2.09 |
Si I | ... | -2.79+-0.31 | 0.82+-0.31 | 4.72 |
Ca I | ... | -3.21+-0.18 | 0.4+-0.18 | 3.13 |
Sc II | ... | -3.67+-0.16 | -0.06+-0.16 | -0.44 |
Ti I | ... | -3.24+-0.16 | 0.37+-0.16 | 1.71 |
Ti II | ... | -3.49+-0.16 | 0.12+-0.16 | 1.54 |
V II | ... | -3.40+-0.31 | 0.21+-0.31 | 0.61 |
Cr I | ... | -3.88+-0.16 | -0.27+-0.16 | 1.76 |
Cr II | ... | -3.77+-0.22 | -0.16+-0.22 | 1.95 |
Mn I | ... | -4.36+-0.14 | -0.75+-0.14 | 1.07 |
Mn II | ... | -4.35+-0.22 | -0.74+-0.22 | 1.16 |
Fe I | ... | -3.61+-0.15 | ... | 3.89 |
Fe II | ... | -3.53+-0.17 | ... | 3.97 |
Co I | ... | -3.37+-0.2 | 0.24+-0.2 | 1.62 |
Ni I | ... | -3.57+-0.22 | 0.04+-0.22 | 2.65 |
Zn I | ... | -3.08+-0.18 | 0.53+-0.18 | 1.48 |
Rb I | ... | <-0.76 | <2.85 | <1.84 |
Sr II | ... | -5.42+-0.15 | -1.81+-0.15 | -2.47 |
Y II | ... | <-4.48 | <-0.87 | <-2.24 |
Zr II | ... | <-3.34 | <0.27 | <-0.74 |
Nb II | ... | <-1.23 | <2.38 | <0.19 |
Mo I | ... | <-2.36 | <1.25 | <-0.44 |
Tc I | ... | <-0.18 | <3.43 | <-0.18 |
Ba II | ... | -4.93+-0.16 | -1.32+-0.16 | -2.67 |
Ce II | ... | <-3.13 | <0.48 | <-1.55 |
Pr II | ... | <-2.54 | <1.07 | <-1.83 |
Nd II | ... | <-3.32 | <0.29 | <-1.82 |
Sm II | ... | <-2.59 | <1.02 | <-1.58 |
Eu II | ... | <-3.15 | <0.46 | <-2.64 |
Gd II | ... | <-2.26 | <1.35 | <-1.14 |
Tb II | ... | <-1.07 | <2.54 | <-1.17 |
Dy II | ... | <-2.94 | <0.67 | <-1.8 |
Ho II | ... | <-2.23 | <1.38 | <-1.97 |
Er II | ... | <-2.62 | <0.99 | <-1.69 |
Tm II | ... | <-2.10 | <1.51 | <-2.1 |
Yb II | ... | <-3.56 | <0.05 | <-2.48 |
Hf II | ... | <-1.77 | <1.84 | <-0.89 |
Pb I | ... | <-1.54 | <2.07 | <0.41 |
Th II | ... | <-1.91 | <1.70 | <-1.91 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)