Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.57-0.2 | +-0.2 | 1.94 |
CH | ... | -2.66+-0.25 | -0.09+-0.25 | 6.01 |
NH | ... | <-2.17 | <0.40 | <5.8 |
O I | ... | -1.85+-0.2 | 0.72+-0.2 | 6.85 |
Mg I | ... | -2.20+-0.22 | 0.37+-0.22 | 5.4 |
Al I | ... | -3.08+-0.32 | -0.51+-0.32 | 3.37 |
Si I | ... | -2.12+-0.36 | 0.45+-0.36 | 5.39 |
K I | ... | -2.25+-0.23 | 0.32+-0.23 | 2.78 |
Ca I | ... | -2.05+-0.22 | 0.52+-0.22 | 4.3 |
Sc II | ... | -2.54+-0.14 | 0.03+-0.14 | 0.85 |
Ti I | ... | -2.08+-0.21 | 0.49+-0.21 | 2.87 |
Ti II | ... | -2.27+-0.14 | 0.3+-0.14 | 2.92 |
Cr I | ... | -2.75+-0.22 | -0.18+-0.22 | 2.89 |
Cr II | ... | -2.25+-0.14 | 0.32+-0.14 | 3.63 |
Mn I | ... | -2.97+-0.21 | -0.4+-0.21 | 2.46 |
Mn II | ... | -3.00+-0.2 | -0.43+-0.2 | 2.67 |
Fe I | ... | -2.57+-0.21 | ... | 4.93 |
Fe II | ... | -2.33+-0.14 | ... | 5.17 |
Co I | ... | -2.57+-0.26 | 0.00+-0.26 | 2.42 |
Ni I | ... | -2.46+-0.27 | 0.11+-0.27 | 3.76 |
Zn I | ... | -2.27+-0.22 | 0.3+-0.22 | 2.29 |
Rb I | ... | <0.07 | <2.64 | <2.67 |
Sr II | ... | -2.34+-0.24 | 0.23+-0.24 | 0.77 |
Y II | ... | -2.90+-0.18 | -0.33+-0.18 | -0.44 |
Zr II | ... | -2.33+-0.16 | 0.24+-0.16 | 0.49 |
Nb II | ... | <-0.06 | <2.51 | <1.36 |
Mo I | ... | <-0.92 | <1.65 | <1 |
Tc I | ... | <1.35 | <3.92 | <1.35 |
Ba II | ... | -3.08+-0.15 | -0.51+-0.15 | -0.65 |
La II | ... | <-2.04 | <0.53 | <-0.87 |
Ce II | ... | <-1.68 | <0.89 | <-0.1 |
Pr II | ... | <-0.85 | <1.72 | <-0.14 |
Nd II | ... | <-1.91 | <0.66 | <-0.41 |
Sm II | ... | <-1.15 | <1.42 | <-0.14 |
Eu II | ... | -1.99+-0.2 | 0.58+-0.2 | -1.22 |
Gd II | ... | <-0.93 | <1.64 | <0.19 |
Tb II | ... | <-0.16 | <2.41 | <-0.26 |
Dy II | ... | -1.48+-0.17 | 1.09+-0.17 | -0.14 |
Er II | ... | <-1.26 | <1.31 | <-0.33 |
Yb II | ... | -2.44+-0.26 | 0.13+-0.26 | -1.28 |
Hf II | ... | <-0.42 | <2.15 | <0.46 |
Pb I | ... | <-0.41 | <2.16 | <1.54 |
Th II | ... | <-0.15 | <2.42 | <-0.15 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)