Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.78-0.2 | +-0.2 | 2 |
CH | ... | -2.20+-0.25 | 0.58+-0.25 | 6.07 |
NH | ... | <-2.07 | <0.71 | <5.9 |
O I | ... | <-2.22 | <0.56 | <6.65 |
Mg I | ... | -2.30+-0.21 | 0.48+-0.21 | 5.31 |
Al I | ... | -3.35+-0.33 | -0.57+-0.33 | 3.1 |
K I | ... | -2.52+-0.23 | 0.26+-0.23 | 2.51 |
Ca I | ... | -2.34+-0.22 | 0.44+-0.22 | 4 |
Sc II | ... | -2.73+-0.16 | 0.05+-0.16 | 0.27 |
Ti I | ... | -2.47+-0.2 | 0.31+-0.2 | 2.49 |
Ti II | ... | -2.47+-0.14 | 0.31+-0.14 | 2.32 |
V I | ... | -2.51+-0.24 | 0.27+-0.24 | 1.42 |
V II | ... | <-2.39 | <0.39 | <1.61 |
Cr I | ... | -2.93+-0.21 | -0.15+-0.21 | 2.72 |
Cr II | ... | -2.37+-0.17 | 0.41+-0.17 | 3.11 |
Mn I | ... | -3.13+-0.21 | -0.35+-0.21 | 2.3 |
Mn II | ... | -3.11+-0.22 | -0.33+-0.22 | 2.16 |
Fe I | ... | -2.78+-0.21 | ... | 4.72 |
Fe II | ... | -2.94+-0.15 | ... | 4.56 |
Co I | ... | -2.62+-0.24 | 0.16+-0.24 | 2.37 |
Ni I | ... | -2.79+-0.29 | -0.01+-0.29 | 3.44 |
Zn I | ... | -2.49+-0.23 | 0.29+-0.23 | 2.07 |
Rb I | ... | <0.09 | <2.87 | <2.69 |
Sr II | ... | -2.56+-0.24 | 0.22+-0.24 | 0.15 |
Y II | ... | -2.87+-0.19 | -0.09+-0.19 | -0.81 |
Zr II | ... | -2.16+-0.16 | 0.62+-0.16 | 0.26 |
Mo I | ... | <-1.05 | <1.73 | <0.87 |
Tc I | ... | <1.12 | <3.90 | <1.12 |
Ba II | ... | -3.12+-0.14 | -0.34+-0.14 | -1.1 |
Ce II | ... | <-1.82 | <0.96 | <-0.24 |
Pr II | ... | <-1.23 | <1.55 | <-0.52 |
Nd II | ... | <-1.93 | <0.85 | <-0.43 |
Sm II | ... | <-1.31 | <1.47 | <-0.3 |
Eu II | ... | <-1.89 | <0.89 | <-1.38 |
Gd II | ... | <-1.11 | <1.67 | <0.01 |
Tb II | ... | <0.21 | <2.99 | <0.11 |
Dy II | ... | <-1.62 | <1.16 | <-0.48 |
Er II | ... | <-1.38 | <1.40 | <-0.45 |
Tm II | ... | <-0.77 | <2.01 | <-0.77 |
Yb II | ... | <-2.39 | <0.39 | <-1.31 |
Hf II | ... | <-0.53 | <2.25 | <0.35 |
Pb I | ... | <-0.48 | <2.30 | <1.47 |
Th II | ... | <-0.41 | <2.37 | <-0.41 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)