Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.44-0.2 | +-0.2 | 2.11 |
CH | ... | -2.48+-0.25 | -0.04+-0.25 | 6.13 |
NH | ... | <-1.47 | <0.97 | <6.5 |
O I | ... | -1.94+-0.2 | 0.5+-0.2 | 6.76 |
Mg I | ... | -2.02+-0.22 | 0.42+-0.22 | 5.58 |
Al I | ... | -3.19+-0.32 | -0.75+-0.32 | 3.27 |
K I | ... | -1.79+-0.23 | 0.65+-0.23 | 3.24 |
Ca I | ... | -1.87+-0.22 | 0.57+-0.22 | 4.47 |
Sc II | ... | -2.23+-0.15 | 0.21+-0.15 | 1.1 |
Ti I | ... | -2.03+-0.2 | 0.41+-0.2 | 2.92 |
Ti II | ... | -1.98+-0.14 | 0.46+-0.14 | 3.14 |
V I | ... | -2.31+-0.26 | 0.13+-0.26 | 1.62 |
V II | ... | -2.22+-0.26 | 0.22+-0.26 | 1.89 |
Cr I | ... | -2.54+-0.21 | -0.1+-0.21 | 3.1 |
Cr II | ... | -2.24+-0.15 | 0.2+-0.15 | 3.58 |
Mn I | ... | -2.77+-0.21 | -0.33+-0.21 | 2.66 |
Mn II | ... | -2.78+-0.21 | -0.34+-0.21 | 2.82 |
Fe I | ... | -2.44+-0.2 | ... | 5.06 |
Fe II | ... | -2.26+-0.15 | ... | 5.24 |
Co I | ... | -2.39+-0.26 | 0.05+-0.26 | 2.6 |
Ni I | ... | -2.38+-0.28 | 0.06+-0.28 | 3.84 |
Cu I | ... | <-1.80 | <0.64 | <2.41 |
Zn I | ... | -2.03+-0.21 | 0.41+-0.21 | 2.53 |
Rb I | ... | <0.27 | <2.71 | <2.87 |
Sr II | ... | -2.18+-0.24 | 0.26+-0.24 | 0.87 |
Y II | ... | -2.68+-0.17 | -0.24+-0.17 | -0.29 |
Zr II | ... | -2.10+-0.14 | 0.34+-0.14 | 0.66 |
Nb II | ... | <0.01 | <2.45 | <1.43 |
Mo I | ... | <-0.80 | <1.64 | <1.12 |
Tc I | ... | <1.41 | <3.85 | <1.41 |
Ba II | ... | -2.84+-0.14 | -0.4+-0.14 | -0.49 |
La II | ... | <-1.70 | <0.74 | <-0.53 |
Ce II | ... | <-1.68 | <0.76 | <-0.1 |
Pr II | ... | <-0.86 | <1.58 | <-0.15 |
Nd II | ... | <-1.77 | <0.67 | <-0.27 |
Sm II | ... | <-1.09 | <1.35 | <-0.08 |
Eu II | ... | <-1.58 | <0.86 | <-1.07 |
Gd II | ... | <-1.08 | <1.36 | <0.04 |
Tb II | ... | <-0.22 | <2.22 | <-0.32 |
Dy II | ... | <-1.32 | <1.12 | <-0.18 |
Er II | ... | <-1.02 | <1.42 | <-0.09 |
Tm II | ... | <-0.71 | <1.73 | <-0.71 |
Yb II | ... | -2.44+-0.39 | 0.00+-0.39 | -1.34 |
Hf II | ... | <-0.35 | <2.09 | <0.53 |
Pb I | ... | <-0.55 | <1.89 | <1.4 |
Th II | ... | <-0.32 | <2.12 | <-0.32 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)