Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-0.78 | <2.49 | <0.38 |
CH | ... | -3.26+-0.25 | 0.01+-0.25 | 5.28 |
NH | ... | <-2.67 | <0.60 | <5.3 |
O I | ... | <-2.44 | <0.83 | <6.43 |
Mg I | ... | -2.74+-0.16 | 0.53+-0.16 | 4.86 |
Al I | ... | -3.76+-0.3 | -0.49+-0.3 | 2.69 |
K I | ... | -2.95+-0.19 | 0.32+-0.19 | 2.08 |
Ca I | ... | -2.82+-0.17 | 0.45+-0.17 | 3.52 |
Sc II | ... | -3.38+-0.15 | -0.11+-0.15 | -0.11 |
Ti I | ... | -3.04+-0.14 | 0.23+-0.14 | 1.91 |
Ti II | ... | -3.09+-0.14 | 0.18+-0.14 | 1.98 |
V I | ... | -3.58+-0.19 | -0.31+-0.19 | 0.35 |
V II | ... | -3.33+-0.24 | -0.06+-0.24 | 0.71 |
Cr I | ... | -3.59+-0.15 | -0.32+-0.15 | 2.05 |
Mn I | ... | -3.86+-0.16 | -0.59+-0.16 | 1.57 |
Mn II | ... | -3.85+-0.23 | -0.58+-0.23 | 1.69 |
Fe I | ... | -3.27+-0.15 | ... | 4.23 |
Fe II | ... | -3.16+-0.15 | ... | 4.34 |
Co I | ... | -3.23+-0.2 | 0.04+-0.2 | 1.76 |
Ni I | ... | -3.19+-0.19 | 0.08+-0.19 | 3.03 |
Zn I | ... | -3.10+-0.17 | 0.17+-0.17 | 1.46 |
Rb I | ... | <-0.98 | <2.29 | <1.62 |
Sr II | ... | -3.36+-0.24 | -0.09+-0.24 | -0.38 |
Y II | ... | -3.95+-0.18 | -0.68+-0.18 | -1.63 |
Zr II | ... | -3.31+-0.16 | -0.04+-0.16 | -0.61 |
Nb II | ... | <-1.48 | <1.79 | <-0.06 |
Mo I | ... | <-2.08 | <1.19 | <-0.16 |
Tc I | ... | <-0.25 | <3.02 | <-0.25 |
Sn I | ... | <-0.84 | <2.43 | <1.16 |
Ba II | ... | -3.82+-0.15 | -0.55+-0.15 | -1.52 |
La II | ... | -3.41+-0.2 | -0.14+-0.2 | -2.2 |
Ce II | ... | <-3.24 | <0.03 | <-1.66 |
Pr II | ... | <-2.41 | <0.86 | <-1.7 |
Nd II | ... | -3.18+-0.16 | 0.09+-0.16 | -1.65 |
Sm II | ... | -2.92+-0.18 | 0.35+-0.18 | -1.85 |
Eu II | ... | -3.11+-0.16 | 0.16+-0.16 | -2.47 |
Gd II | ... | <-2.18 | <1.09 | <-1.06 |
Tb II | ... | <-1.94 | <1.33 | <-2.04 |
Dy II | ... | -3.20+-0.17 | 0.07+-0.17 | -1.99 |
Er II | ... | -3.01+-0.18 | 0.26+-0.18 | -1.98 |
Tm II | ... | <-2.25 | <1.02 | <-2.25 |
Yb II | ... | -3.39+-0.19 | -0.12+-0.19 | -2.36 |
Hf II | ... | <-1.78 | <1.49 | <-0.9 |
Pb I | ... | <-1.95 | <1.32 | <0 |
Th II | ... | <-1.96 | <1.31 | <-1.96 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)