Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.85-0.2 | +-0.2 | 2.02 |
CH | ... | -2.93+-0.25 | -0.08+-0.25 | 5.76 |
NH | ... | <-2.12 | <0.73 | <5.85 |
O I | ... | -1.98+-0.2 | 0.87+-0.2 | 6.71 |
Mg I | ... | -2.37+-0.21 | 0.48+-0.21 | 5.23 |
Al I | ... | -3.53+-0.29 | -0.68+-0.29 | 2.91 |
Si I | ... | -2.41+-0.36 | 0.44+-0.36 | 5.1 |
Ca I | ... | -2.36+-0.22 | 0.49+-0.22 | 3.98 |
Sc II | ... | -2.91+-0.15 | -0.06+-0.15 | 0.51 |
Ti I | ... | -2.41+-0.2 | 0.44+-0.2 | 2.54 |
Ti II | ... | -2.54+-0.15 | 0.31+-0.15 | 2.67 |
V II | ... | <-2.35 | <0.50 | <1.65 |
Cr I | ... | -2.98+-0.21 | -0.13+-0.21 | 2.66 |
Cr II | ... | -2.54+-0.15 | 0.31+-0.15 | 3.36 |
Mn I | ... | -3.26+-0.2 | -0.41+-0.2 | 2.17 |
Mn II | ... | -3.36+-0.21 | -0.51+-0.21 | 2.33 |
Fe I | ... | -2.85+-0.21 | ... | 4.65 |
Fe II | ... | -2.59+-0.15 | ... | 4.91 |
Co I | ... | -2.79+-0.25 | 0.06+-0.25 | 2.2 |
Ni I | ... | -2.95+-0.26 | -0.1+-0.26 | 3.27 |
Zn I | ... | <-2.35 | <0.50 | <2.25 |
Rb I | ... | <-0.03 | <2.82 | <2.57 |
Sr II | ... | -2.85+-0.23 | 0.00+-0.23 | 0.28 |
Y II | ... | -3.27+-0.22 | -0.42+-0.22 | -0.8 |
Zr II | ... | <-2.24 | <0.61 | <0.36 |
Nb II | ... | <-0.15 | <2.70 | <1.27 |
Mo I | ... | <-1.08 | <1.77 | <0.84 |
Tc I | ... | <1.23 | <4.08 | <1.23 |
Ba II | ... | -3.64+-0.14 | -0.79+-0.14 | -1.2 |
Ce II | ... | <-1.66 | <1.19 | <-0.08 |
Pr II | ... | <-1.29 | <1.56 | <-0.58 |
Nd II | ... | <-1.80 | <1.05 | <-0.3 |
Sm II | ... | <-1.13 | <1.72 | <-0.12 |
Eu II | ... | <-1.69 | <1.16 | <-1.18 |
Gd II | ... | <-1.01 | <1.84 | <0.11 |
Tb II | ... | <-0.37 | <2.48 | <-0.47 |
Dy II | ... | <-1.69 | <1.16 | <-0.55 |
Ho II | ... | <-0.99 | <1.86 | <-0.73 |
Er II | ... | <-1.44 | <1.41 | <-0.51 |
Tm II | ... | <-0.77 | <2.08 | <-0.77 |
Yb II | ... | <-2.31 | <0.54 | <-1.23 |
Hf II | ... | <-0.57 | <2.28 | <0.31 |
Pb I | ... | <-0.50 | <2.35 | <1.45 |
Th II | ... | <-0.44 | <2.41 | <-0.44 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)