Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.78-0.2 | +-0.2 | 1.96 |
CH | ... | -2.38+-0.25 | 0.4+-0.25 | 6.23 |
NH | ... | <-1.12 | <1.66 | <6.85 |
O I | ... | -2.29+-0.2 | 0.49+-0.2 | 6.4 |
Mg I | ... | -2.43+-0.22 | 0.35+-0.22 | 5.17 |
Al I | ... | -3.60+-0.23 | -0.82+-0.23 | 2.85 |
Si I | ... | -2.51+-0.36 | 0.27+-0.36 | 5 |
Ca I | ... | -2.33+-0.22 | 0.45+-0.22 | 4.01 |
Sc II | ... | -2.75+-0.15 | 0.03+-0.15 | 0.58 |
Ti I | ... | -2.44+-0.22 | 0.34+-0.22 | 2.51 |
Ti II | ... | -2.56+-0.14 | 0.22+-0.14 | 2.57 |
V II | ... | -2.31+-0.28 | 0.47+-0.28 | 1.8 |
Cr I | ... | -2.90+-0.2 | -0.12+-0.2 | 2.74 |
Cr II | ... | -2.67+-0.17 | 0.11+-0.17 | 3.15 |
Mn I | ... | -3.01+-0.22 | -0.23+-0.22 | 2.42 |
Mn II | ... | -3.20+-0.2 | -0.42+-0.2 | 2.41 |
Fe I | ... | -2.78+-0.21 | ... | 4.72 |
Fe II | ... | -2.6+-0.15 | ... | 4.9 |
Co I | ... | -2.60+-0.24 | 0.18+-0.24 | 2.39 |
Ni I | ... | -2.77+-0.25 | 0.01+-0.25 | 3.45 |
Zn I | ... | <-2.07 | <0.71 | <2.53 |
Rb I | ... | <0.32 | <3.10 | <2.92 |
Sr II | ... | -3.63+-0.14 | -0.85+-0.14 | -0.58 |
Y II | ... | <-2.25 | <0.53 | <-0.01 |
Zr II | ... | <-1.65 | <1.13 | <0.95 |
Nb II | ... | <0.09 | <2.87 | <1.51 |
Mo I | ... | <-0.58 | <2.20 | <1.34 |
Tc I | ... | <1.51 | <4.29 | <1.51 |
Ba II | ... | <-3.61 | <-0.83 | <-1.48 |
La II | ... | <-1.68 | <1.10 | <-0.51 |
Ce II | ... | <-1.36 | <1.42 | <0.22 |
Pr II | ... | <-0.85 | <1.93 | <-0.14 |
Nd II | ... | <-1.49 | <1.29 | <0.01 |
Sm II | ... | <-0.89 | <1.89 | <0.12 |
Eu II | ... | <-1.61 | <1.17 | <-1.1 |
Gd II | ... | <-0.85 | <1.93 | <0.27 |
Tb II | ... | <0.01 | <2.79 | <-0.09 |
Dy II | ... | <-0.80 | <1.98 | <0.34 |
Ho II | ... | <-0.58 | <2.20 | <-0.32 |
Er II | ... | <-0.93 | <1.85 | <0 |
Tm II | ... | <-0.33 | <2.45 | <-0.33 |
Hf II | ... | <-0.34 | <2.44 | <0.54 |
Pb I | ... | <-0.26 | <2.52 | <1.69 |
Th II | ... | <-0.27 | <2.51 | <-0.27 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)