Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.73-0.2 | +-0.2 | 1.98 |
CH | ... | -2.68+-0.25 | 0.05+-0.25 | 5.91 |
NH | ... | <-1.77 | <0.96 | <6.2 |
O I | ... | -1.97+-0.2 | 0.76+-0.2 | 6.72 |
Mg I | ... | -2.32+-0.21 | 0.41+-0.21 | 5.29 |
Al I | ... | -3.56+-0.3 | -0.83+-0.3 | 2.89 |
Si I | ... | -2.14+-0.36 | 0.59+-0.36 | 5.37 |
K I | ... | -2.41+-0.24 | 0.32+-0.24 | 2.62 |
Ca I | ... | -2.23+-0.22 | 0.5+-0.22 | 4.11 |
Sc II | ... | -2.68+-0.14 | 0.05+-0.14 | 0.63 |
Ti I | ... | -2.36+-0.2 | 0.37+-0.2 | 2.6 |
Ti II | ... | -2.53+-0.15 | 0.2+-0.15 | 2.58 |
V II | ... | <-2.16 | <0.57 | <1.84 |
Cr I | ... | -2.94+-0.21 | -0.21+-0.21 | 2.7 |
Cr II | ... | -2.47+-0.16 | 0.26+-0.16 | 3.32 |
Mn I | ... | -3.07+-0.2 | -0.34+-0.2 | 2.36 |
Mn II | ... | -3.29+-0.2 | -0.56+-0.2 | 2.3 |
Fe I | ... | -2.73+-0.21 | ... | 4.77 |
Fe II | ... | -2.57+-0.14 | ... | 4.93 |
Co I | ... | -2.67+-0.24 | 0.06+-0.24 | 2.32 |
Ni I | ... | -2.74+-0.27 | -0.01+-0.27 | 3.48 |
Zn I | ... | <-2.14 | <0.59 | <2.46 |
Rb I | ... | <0.29 | <3.02 | <2.89 |
Sr II | ... | -2.97+-0.23 | -0.24+-0.23 | 0.06 |
Zr II | ... | -2.58+-0.17 | 0.15+-0.17 | 0.16 |
Nb II | ... | <0.61 | <3.34 | <2.03 |
Mo I | ... | <-0.77 | <1.96 | <1.15 |
Tc I | ... | <1.42 | <4.15 | <1.42 |
Ba II | ... | -3.35+-0.15 | -0.62+-0.15 | -1.01 |
Ce II | ... | <-1.37 | <1.36 | <0.21 |
Pr II | ... | <-0.91 | <1.82 | <-0.2 |
Nd II | ... | <-1.71 | <1.02 | <-0.21 |
Sm II | ... | <-1.07 | <1.66 | <-0.06 |
Eu II | ... | <-1.71 | <1.02 | <-1.2 |
Gd II | ... | <-0.87 | <1.86 | <0.25 |
Tb II | ... | <-0.01 | <2.72 | <-0.11 |
Dy II | ... | <-1.38 | <1.35 | <-0.24 |
Ho II | ... | <-0.69 | <2.04 | <-0.43 |
Er II | ... | <-1.04 | <1.69 | <-0.11 |
Tm II | ... | <-0.25 | <2.48 | <-0.25 |
Yb II | ... | <-2.27 | <0.46 | <-1.19 |
Hf II | ... | <-0.39 | <2.34 | <0.49 |
Pb I | ... | <-0.30 | <2.43 | <1.65 |
Th II | ... | <-0.33 | <2.40 | <-0.33 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)