Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.84 | <3.48 | <2 |
CH | ... | <-1.05 | <1.59 | <7.5 |
CN | ... | <0.18 | <2.82 | <8.15 |
O I | ... | -2.89+-0.17 | -0.25+-0.17 | 5.8 |
Mg I | ... | -2.41+-0.18 | 0.23+-0.18 | 5.19 |
Al I | ... | -3.32+-0.18 | -0.68+-0.18 | 3.13 |
Si I | ... | -2.51+-0.27 | 0.13+-0.27 | 5 |
Ca I | ... | -2.11+-0.19 | 0.53+-0.19 | 4.23 |
Sc II | ... | -2.54+-0.16 | 0.1+-0.16 | 0.6 |
Ti I | ... | -2.29+-0.23 | 0.35+-0.23 | 2.66 |
Ti II | ... | -2.26+-0.15 | 0.38+-0.15 | 2.68 |
V II | ... | -2.32+-0.26 | 0.32+-0.26 | 1.6 |
Cr I | ... | -2.68+-0.17 | -0.04+-0.17 | 2.95 |
Cr II | ... | -2.40+-0.16 | 0.24+-0.16 | 3.23 |
Mn I | ... | -2.70+-0.19 | -0.06+-0.19 | 2.73 |
Mn II | ... | -2.82+-0.21 | -0.18+-0.21 | 2.6 |
Fe I | ... | -2.64+-0.17 | ... | 4.86 |
Fe II | ... | -2.65+-0.16 | ... | 4.85 |
Co I | ... | -2.40+-0.22 | 0.24+-0.22 | 2.59 |
Ni I | ... | -2.46+-0.22 | 0.18+-0.22 | 3.76 |
Rb I | ... | <0.56 | <3.20 | <3.16 |
Sr II | ... | -3.11+-0.18 | -0.47+-0.18 | -0.25 |
Zr II | ... | <-2.29 | <0.35 | <0.31 |
Nb II | ... | <-0.31 | <2.33 | <1.11 |
Mo I | ... | <-0.21 | <2.43 | <1.71 |
Tc I | ... | <1.97 | <4.61 | <1.97 |
Ba II | ... | -3.39+-0.15 | -0.75+-0.15 | -1.22 |
Ce II | ... | <-1.44 | <1.20 | <0.14 |
Pr II | ... | <-0.99 | <1.65 | <-0.28 |
Nd II | ... | <-1.66 | <0.98 | <-0.16 |
Sm II | ... | <-1.18 | <1.46 | <-0.17 |
Eu II | ... | <-1.64 | <1.00 | <-1.13 |
Gd II | ... | <-1.03 | <1.61 | <0.09 |
Tb II | ... | <-0.22 | <2.42 | <-0.32 |
Dy II | ... | <-1.56 | <1.08 | <-0.42 |
Ho II | ... | <-0.99 | <1.65 | <-0.73 |
Er II | ... | <-1.11 | <1.53 | <-0.18 |
Tm II | ... | <-0.73 | <1.91 | <-0.73 |
Yb II | ... | <-2.10 | <0.54 | <-1.02 |
Hf II | ... | <-0.31 | <2.33 | <0.57 |
Pb I | ... | <0.11 | <2.75 | <2.06 |
Th II | ... | <-0.30 | <2.34 | <-0.3 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)