Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.51-0.15 | +-0.15 | 1.08 |
CH | ... | -3.16+-0.25 | 0.35+-0.25 | 5.32 |
NH | ... | <-2.37 | <1.14 | <5.6 |
O I | ... | <-2.30 | <1.21 | <6.57 |
Mg I | ... | -2.97+-0.15 | 0.54+-0.15 | 4.64 |
Al I | ... | -4.22+-0.2 | -0.71+-0.2 | 2.23 |
Si I | ... | -2.69+-0.32 | 0.82+-0.32 | 4.82 |
Ca I | ... | -2.99+-0.17 | 0.52+-0.17 | 3.36 |
Sc II | ... | -3.68+-0.16 | -0.17+-0.16 | -0.48 |
Ti I | ... | -3.18+-0.15 | 0.33+-0.15 | 1.77 |
Ti II | ... | -3.32+-0.15 | 0.19+-0.15 | 1.69 |
Cr I | ... | -3.81+-0.14 | -0.3+-0.14 | 1.83 |
Mn I | ... | -3.95+-0.14 | -0.44+-0.14 | 1.48 |
Mn II | ... | -4.10+-0.23 | -0.59+-0.23 | 1.38 |
Fe I | ... | -3.51+-0.15 | ... | 3.99 |
Fe II | ... | -3.45+-0.17 | ... | 4.05 |
Co I | ... | -3.31+-0.21 | 0.2+-0.21 | 1.68 |
Ni I | ... | -3.46+-0.22 | 0.05+-0.22 | 2.77 |
Zn I | ... | -2.85+-0.18 | 0.66+-0.18 | 1.71 |
Rb I | ... | <-0.55 | <2.96 | <2.05 |
Sr II | ... | -3.71+-0.18 | -0.2+-0.18 | -0.78 |
Y II | ... | -3.95+-0.22 | -0.44+-0.22 | -1.68 |
Zr II | ... | <-3.40 | <0.11 | <-0.8 |
Mo I | ... | <-1.96 | <1.55 | <-0.04 |
Ba II | ... | -4.37+-0.15 | -0.86+-0.15 | -2.13 |
Ce II | ... | <-2.57 | <0.94 | <-0.99 |
Pr II | ... | <-2.29 | <1.22 | <-1.58 |
Nd II | ... | <-2.38 | <1.13 | <-0.88 |
Sm II | ... | <-2.27 | <1.24 | <-1.26 |
Eu II | ... | <-2.95 | <0.56 | <-2.44 |
Gd II | ... | <-1.96 | <1.55 | <-0.84 |
Tb II | ... | <-1.37 | <2.14 | <-1.47 |
Dy II | ... | <-2.66 | <0.85 | <-1.52 |
Er II | ... | <-2.30 | <1.21 | <-1.37 |
Tm II | ... | <-1.70 | <1.81 | <-1.7 |
Yb II | ... | <-3.48 | <0.03 | <-2.4 |
Hf II | ... | <-1.47 | <2.04 | <-0.59 |
Pb I | ... | <-1.22 | <2.29 | <0.73 |
Th II | ... | <-1.64 | <1.87 | <-1.64 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)