Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.03-0.2 | +-0.2 | 2.04 |
CH | ... | <-2.55 | <0.48 | <6 |
NH | ... | <-1.62 | <1.41 | <6.35 |
O I | ... | <-2.63 | <0.40 | <6.24 |
Mg I | ... | -2.58+-0.21 | 0.45+-0.21 | 5.02 |
Al I | ... | -3.45+-0.28 | -0.42+-0.28 | 3 |
Si I | ... | -2.50+-0.36 | 0.53+-0.36 | 5.01 |
Ca I | ... | -2.46+-0.22 | 0.57+-0.22 | 3.88 |
Sc II | ... | -3.06+-0.15 | -0.03+-0.15 | 0.35 |
Ti I | ... | -2.52+-0.22 | 0.51+-0.22 | 2.43 |
Ti II | ... | -2.77+-0.15 | 0.26+-0.15 | 2.44 |
V II | ... | <-2.28 | <0.75 | <1.72 |
Cr I | ... | -3.20+-0.2 | -0.17+-0.2 | 2.43 |
Cr II | ... | -2.73+-0.16 | 0.3+-0.16 | 3.17 |
Mn I | ... | -3.44+-0.21 | -0.41+-0.21 | 1.99 |
Mn II | ... | -3.42+-0.22 | -0.39+-0.22 | 2.27 |
Fe I | ... | -3.03+-0.22 | ... | 4.47 |
Fe II | ... | -2.77+-0.15 | ... | 4.73 |
Co I | ... | -2.81+-0.24 | 0.22+-0.24 | 2.18 |
Ni I | ... | -2.98+-0.26 | 0.05+-0.26 | 3.24 |
Zn I | ... | <-2.18 | <0.85 | <2.42 |
Rb I | ... | <0.39 | <3.42 | <2.99 |
Sr II | ... | -3.24+-0.19 | -0.21+-0.19 | -0.11 |
Y II | ... | -3.29+-0.24 | -0.26+-0.24 | -0.82 |
Zr II | ... | <-2.43 | <0.60 | <0.17 |
Nb II | ... | <-0.01 | <3.02 | <1.41 |
Mo I | ... | <-0.87 | <2.16 | <1.05 |
Tc I | ... | <1.34 | <4.37 | <1.34 |
Ba II | ... | -3.80+-0.15 | -0.77+-0.15 | -1.36 |
La II | ... | <-1.87 | <1.16 | <-0.7 |
Ce II | ... | <-1.62 | <1.41 | <-0.04 |
Pr II | ... | <-1.12 | <1.91 | <-0.41 |
Nd II | ... | <-1.75 | <1.28 | <-0.25 |
Sm II | ... | <-1.20 | <1.83 | <-0.19 |
Eu II | ... | <-1.87 | <1.16 | <-1.36 |
Gd II | ... | <-1.03 | <2.00 | <0.09 |
Tb II | ... | <-0.20 | <2.83 | <-0.3 |
Dy II | ... | <-1.49 | <1.54 | <-0.35 |
Ho II | ... | <-0.83 | <2.20 | <-0.57 |
Er II | ... | <-1.28 | <1.75 | <-0.35 |
Tm II | ... | <-0.61 | <2.42 | <-0.61 |
Yb II | ... | <-2.33 | <0.70 | <-1.25 |
Hf II | ... | <-0.36 | <2.67 | <0.52 |
Pb I | ... | <-0.36 | <2.67 | <1.59 |
Th II | ... | <-0.34 | <2.69 | <-0.34 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)