Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.63-0.2 | +-0.2 | 2.08 |
CH | ... | -1.94+-0.25 | 0.69+-0.25 | 6.45 |
NH | ... | -2.14+-0.36 | 0.49+-0.36 | 5.65 |
O I | ... | <-2.34 | <0.29 | <6.53 |
Mg I | ... | -2.11+-0.23 | 0.52+-0.23 | 5.5 |
Al I | ... | -3.28+-0.33 | -0.65+-0.33 | 3.17 |
Si I | ... | -1.87+-0.37 | 0.76+-0.37 | 5.64 |
Ca I | ... | -2.14+-0.22 | 0.49+-0.22 | 4.2 |
Sc II | ... | -2.62+-0.15 | 0.01+-0.15 | 0.48 |
Ti I | ... | -2.27+-0.2 | 0.36+-0.2 | 2.68 |
Ti II | ... | -2.33+-0.14 | 0.3+-0.14 | 2.58 |
V I | ... | -2.50+-0.25 | 0.13+-0.25 | 1.43 |
V II | ... | <-2.30 | <0.33 | <1.7 |
Cr I | ... | -2.81+-0.21 | -0.18+-0.21 | 2.83 |
Cr II | ... | -2.59+-0.25 | 0.04+-0.25 | 3.01 |
Mn I | ... | -3.00+-0.21 | -0.37+-0.21 | 2.44 |
Mn II | ... | -2.95+-0.2 | -0.32+-0.2 | 2.43 |
Fe I | ... | -2.63+-0.21 | ... | 4.87 |
Fe II | ... | -2.67+-0.15 | ... | 4.83 |
Co I | ... | -2.48+-0.25 | 0.15+-0.25 | 2.52 |
Ni I | ... | -2.60+-0.29 | 0.03+-0.29 | 3.62 |
Zn I | ... | -2.59+-0.26 | 0.04+-0.26 | 1.97 |
Rb I | ... | <0.26 | <2.89 | <2.86 |
Sr II | ... | -2.36+-0.24 | 0.27+-0.24 | 0.46 |
Y II | ... | -2.73+-0.18 | -0.1+-0.18 | -0.56 |
Zr II | ... | -2.12+-0.2 | 0.51+-0.2 | 0.41 |
Nb II | ... | <-0.13 | <2.50 | <1.29 |
Mo I | ... | <-1.12 | <1.51 | <0.8 |
Tc I | ... | <1.35 | <3.98 | <1.35 |
Ba II | ... | -2.68+-0.14 | -0.05+-0.14 | -0.54 |
Ce II | ... | <-1.28 | <1.35 | <0.3 |
Pr II | ... | <-1.14 | <1.49 | <-0.43 |
Nd II | ... | <-1.72 | <0.91 | <-0.22 |
Sm II | ... | <-1.35 | <1.28 | <-0.34 |
Eu II | ... | -1.77+-0.22 | 0.86+-0.22 | -1.29 |
Gd II | ... | <-0.85 | <1.78 | <0.27 |
Tb II | ... | <-0.41 | <2.22 | <-0.51 |
Dy II | ... | <-1.47 | <1.16 | <-0.33 |
Er II | ... | <-1.23 | <1.40 | <-0.3 |
Tm II | ... | <-0.74 | <1.89 | <-0.74 |
Yb II | ... | -2.26+-0.32 | 0.37+-0.32 | -1.38 |
Hf II | ... | <-0.56 | <2.07 | <0.32 |
Pb I | ... | <-0.40 | <2.23 | <1.55 |
Th II | ... | <-0.52 | <2.11 | <-0.52 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)