Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.96-0.2 | +-0.2 | 1.98 |
CH | ... | <-2.45 | <0.51 | <6.1 |
CN | ... | <-0.07 | <2.89 | <7.9 |
O I | ... | <-2.61 | <0.35 | <6.26 |
Mg I | ... | -2.73+-0.21 | 0.23+-0.21 | 4.87 |
Al I | ... | -3.81+-0.22 | -0.85+-0.22 | 2.64 |
Si I | ... | -2.64+-0.36 | 0.32+-0.36 | 4.87 |
Ca I | ... | -2.52+-0.22 | 0.44+-0.22 | 3.82 |
Sc II | ... | -3.00+-0.15 | -0.04+-0.15 | 0.38 |
Ti I | ... | -2.53+-0.21 | 0.43+-0.21 | 2.41 |
Ti II | ... | -2.71+-0.14 | 0.25+-0.14 | 2.48 |
V II | ... | <-2.27 | <0.69 | <1.73 |
Cr I | ... | -3.15+-0.2 | -0.19+-0.2 | 2.48 |
Cr II | ... | -2.68+-0.16 | 0.28+-0.16 | 3.2 |
Mn I | ... | -3.26+-0.22 | -0.3+-0.22 | 2.17 |
Mn II | ... | -3.36+-0.21 | -0.4+-0.21 | 2.3 |
Fe I | ... | -2.96+-0.21 | ... | 4.54 |
Fe II | ... | -2.73+-0.15 | ... | 4.77 |
Co I | ... | -2.90+-0.26 | 0.06+-0.26 | 2.09 |
Ni I | ... | -2.93+-0.26 | 0.03+-0.26 | 3.29 |
Zn I | ... | <-2.28 | <0.68 | <2.32 |
Rb I | ... | <0.32 | <3.28 | <2.92 |
Sr II | ... | -3.20+-0.21 | -0.24+-0.21 | -0.09 |
Y II | ... | -3.33+-0.23 | -0.37+-0.23 | -0.89 |
Nb II | ... | <-0.06 | <2.90 | <1.36 |
Mo I | ... | <-0.73 | <2.23 | <1.19 |
Tc I | ... | <1.46 | <4.42 | <1.46 |
Ba II | ... | -3.66+-0.14 | -0.7+-0.14 | -1.25 |
Ce II | ... | <-1.62 | <1.34 | <-0.04 |
Pr II | ... | <-0.98 | <1.98 | <-0.27 |
Nd II | ... | <-1.66 | <1.30 | <-0.16 |
Sm II | ... | <-1.09 | <1.87 | <-0.08 |
Eu II | ... | <-1.89 | <1.07 | <-1.38 |
Gd II | ... | <-0.96 | <2.00 | <0.16 |
Tb II | ... | <-0.16 | <2.80 | <-0.26 |
Dy II | ... | <-1.44 | <1.52 | <-0.3 |
Ho II | ... | <-0.78 | <2.18 | <-0.52 |
Er II | ... | <-1.13 | <1.83 | <-0.2 |
Tm II | ... | <-0.49 | <2.47 | <-0.49 |
Yb II | ... | <-2.40 | <0.56 | <-1.32 |
Hf II | ... | <-0.23 | <2.73 | <0.65 |
Pb I | ... | <-0.38 | <2.58 | <1.57 |
Th II | ... | <-0.30 | <2.66 | <-0.3 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)