Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.97-0.16 | +-0.16 | 0.8 |
CH | ... | -2.83+-0.25 | 0.14+-0.25 | 5.59 |
NH | ... | <-2.77 | <0.20 | <5.2 |
O I | ... | <-2.22 | <0.75 | <6.65 |
Mg I | ... | -2.49+-0.15 | 0.48+-0.15 | 5.11 |
Al I | ... | -3.63+-0.29 | -0.66+-0.29 | 2.82 |
K I | ... | -2.65+-0.18 | 0.32+-0.18 | 2.38 |
Ca I | ... | -2.56+-0.17 | 0.41+-0.17 | 3.77 |
Sc II | ... | -3.03+-0.15 | -0.06+-0.15 | 0.12 |
Ti I | ... | -2.83+-0.15 | 0.14+-0.15 | 2.12 |
Ti II | ... | -2.78+-0.15 | 0.19+-0.15 | 2.17 |
V I | ... | -3.08+-0.18 | -0.11+-0.18 | 0.85 |
V II | ... | -2.89+-0.24 | 0.08+-0.24 | 1.03 |
Cr I | ... | -3.16+-0.15 | -0.19+-0.15 | 2.48 |
Cr II | ... | -2.72+-0.16 | 0.25+-0.16 | 2.92 |
Mn I | ... | -3.30+-0.15 | -0.33+-0.15 | 2.13 |
Mn II | ... | -3.41+-0.21 | -0.44+-0.21 | 2.02 |
Fe I | ... | -2.97+-0.15 | ... | 4.53 |
Fe II | ... | -2.97+-0.16 | ... | 4.53 |
Co I | ... | -3.02+-0.19 | -0.05+-0.19 | 1.97 |
Ni I | ... | -2.85+-0.19 | 0.12+-0.19 | 3.37 |
Zn I | ... | -2.55+-0.15 | 0.42+-0.15 | 2.01 |
Rb I | ... | <-0.77 | <2.20 | <1.83 |
Sr II | ... | -2.85+-0.25 | 0.12+-0.25 | 0.02 |
Y II | ... | -3.55+-0.19 | -0.58+-0.19 | -1.34 |
Zr II | ... | -2.92+-0.17 | 0.05+-0.17 | -0.34 |
Nb II | ... | <-0.98 | <1.99 | <0.44 |
Mo I | ... | <-1.89 | <1.08 | <0.03 |
Tc I | ... | <0.44 | <3.41 | <0.44 |
Ba II | ... | -3.62+-0.15 | -0.65+-0.15 | -1.44 |
La II | ... | <-3.08 | <-0.11 | <-1.91 |
Ce II | ... | <-2.88 | <0.09 | <-1.3 |
Pr II | ... | <-2.41 | <0.56 | <-1.7 |
Nd II | ... | <-2.74 | <0.23 | <-1.24 |
Eu II | ... | -2.95+-0.18 | 0.02+-0.18 | -2.43 |
Gd II | ... | <-2.06 | <0.91 | <-0.94 |
Tb II | ... | <-1.50 | <1.47 | <-1.6 |
Dy II | ... | -2.87+-0.24 | 0.1+-0.24 | -1.77 |
Er II | ... | <-2.36 | <0.61 | <-1.43 |
Tm II | ... | <-1.85 | <1.12 | <-1.85 |
Yb II | ... | -3.24+-0.24 | -0.27+-0.24 | -2.32 |
Hf II | ... | <-1.62 | <1.35 | <-0.74 |
Pb I | ... | <-1.19 | <1.78 | <0.76 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)