Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.29-0.2 | +-0.2 | 1.95 |
CH | ... | <-2.65 | <0.64 | <5.9 |
NH | ... | <-2.07 | <1.22 | <5.9 |
O I | ... | <-2.53 | <0.76 | <6.34 |
Mg I | ... | -2.79+-0.21 | 0.5+-0.21 | 4.81 |
Al I | ... | -4.04+-0.22 | -0.75+-0.22 | 2.41 |
Si I | ... | -2.90+-0.36 | 0.39+-0.36 | 4.61 |
Ca I | ... | -2.73+-0.23 | 0.56+-0.23 | 3.61 |
Sc II | ... | -3.31+-0.15 | -0.02+-0.15 | 0.11 |
Ti I | ... | -2.71+-0.21 | 0.58+-0.21 | 2.24 |
Ti II | ... | -3.16+-0.14 | 0.13+-0.14 | 2.05 |
V II | ... | <-2.13 | <1.16 | <1.87 |
Cr I | ... | -3.62+-0.2 | -0.33+-0.2 | 2.02 |
Mn I | ... | -3.84+-0.2 | -0.55+-0.2 | 1.59 |
Mn II | ... | -3.75+-0.2 | -0.46+-0.2 | 1.95 |
Fe I | ... | -3.29+-0.22 | ... | 4.21 |
Fe II | ... | -3.02+-0.14 | ... | 4.48 |
Co I | ... | -3.17+-0.27 | 0.12+-0.27 | 1.82 |
Ni I | ... | -3.51+-0.27 | -0.22+-0.27 | 2.71 |
Zn I | ... | <-2.37 | <0.92 | <2.23 |
Sr II | ... | -3.60+-0.16 | -0.31+-0.16 | -0.46 |
Y II | ... | <-3.20 | <0.09 | <-0.96 |
Zr II | ... | <-2.31 | <0.98 | <0.29 |
Nb II | ... | <-0.10 | <3.19 | <1.32 |
Mo I | ... | <-0.73 | <2.56 | <1.19 |
Tc I | ... | <1.39 | <4.68 | <1.39 |
Ba II | ... | -3.97+-0.15 | -0.68+-0.15 | -1.52 |
La II | ... | <-1.57 | <1.72 | <-0.4 |
Ce II | ... | <-1.55 | <1.74 | <0.03 |
Pr II | ... | <-0.98 | <2.31 | <-0.27 |
Nd II | ... | <-1.67 | <1.62 | <-0.17 |
Sm II | ... | <-1.06 | <2.23 | <-0.05 |
Eu II | ... | <-1.91 | <1.38 | <-1.4 |
Gd II | ... | <-0.85 | <2.44 | <0.27 |
Tb II | ... | <0.35 | <3.64 | <0.25 |
Dy II | ... | <-1.66 | <1.63 | <-0.52 |
Ho II | ... | <-0.80 | <2.49 | <-0.54 |
Er II | ... | <-1.15 | <2.14 | <-0.22 |
Tm II | ... | <-0.70 | <2.59 | <-0.7 |
Yb II | ... | <-1.90 | <1.39 | <-0.82 |
Hf II | ... | <-0.24 | <3.05 | <0.64 |
Ir I | ... | <0.22 | <3.51 | <1.57 |
Pb I | ... | <-0.28 | <3.01 | <1.67 |
Th II | ... | <-0.22 | <3.07 | <-0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)