Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.67-0.2 | +-0.2 | 1.8 |
CH | ... | -2.27+-0.25 | 0.4+-0.25 | 6.21 |
NH | ... | <-2.02 | <0.65 | <5.95 |
O I | ... | <-2.15 | <0.52 | <6.72 |
Mg I | ... | -2.24+-0.22 | 0.43+-0.22 | 5.36 |
Al I | ... | -3.44+-0.31 | -0.77+-0.31 | 3.01 |
Si I | ... | -2.14+-0.36 | 0.53+-0.36 | 5.37 |
K I | ... | -2.35+-0.24 | 0.32+-0.24 | 2.68 |
Ca I | ... | -2.26+-0.22 | 0.41+-0.22 | 4.08 |
Sc II | ... | -2.90+-0.15 | -0.23+-0.15 | 0.3 |
Ti I | ... | -2.40+-0.2 | 0.27+-0.2 | 2.55 |
Ti II | ... | -2.48+-0.15 | 0.19+-0.15 | 2.52 |
Cr I | ... | -2.86+-0.21 | -0.19+-0.21 | 2.78 |
Cr II | ... | -2.49+-0.16 | 0.18+-0.16 | 3.2 |
Mn I | ... | -3.05+-0.22 | -0.38+-0.22 | 2.39 |
Mn II | ... | -3.01+-0.2 | -0.34+-0.2 | 2.47 |
Fe I | ... | -2.67+-0.21 | ... | 4.83 |
Fe II | ... | -2.62+-0.15 | ... | 4.88 |
Co I | ... | -2.61+-0.25 | 0.06+-0.25 | 2.38 |
Ni I | ... | -2.62+-0.28 | 0.05+-0.28 | 3.6 |
Zn I | ... | -2.30+-0.22 | 0.37+-0.22 | 2.26 |
Rb I | ... | <0.16 | <2.83 | <2.76 |
Sr II | ... | -2.58+-0.24 | 0.09+-0.24 | 0.34 |
Y II | ... | -2.86+-0.21 | -0.19+-0.21 | -0.6 |
Zr II | ... | -2.48+-0.17 | 0.19+-0.17 | 0.15 |
Mo I | ... | <-0.95 | <1.72 | <0.97 |
Tc I | ... | <1.34 | <4.01 | <1.34 |
Ba II | ... | -3.26+-0.14 | -0.59+-0.14 | -1.03 |
Ce II | ... | <-1.72 | <0.95 | <-0.14 |
Pr II | ... | <-0.84 | <1.83 | <-0.13 |
Nd II | ... | <-1.11 | <1.56 | <0.39 |
Sm II | ... | <-1.01 | <1.66 | <0 |
Eu II | ... | <-1.77 | <0.90 | <-1.26 |
Gd II | ... | <-0.86 | <1.81 | <0.26 |
Tb II | ... | <-0.25 | <2.42 | <-0.35 |
Dy II | ... | <-1.51 | <1.16 | <-0.37 |
Ho II | ... | <-0.88 | <1.79 | <-0.62 |
Er II | ... | <-1.25 | <1.42 | <-0.32 |
Tm II | ... | <-0.59 | <2.08 | <-0.59 |
Hf II | ... | <-0.41 | <2.26 | <0.47 |
Pb I | ... | <-0.56 | <2.11 | <1.39 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)