Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.83-0.2 | +-0.2 | 2.2 |
CH | ... | -1.95+-0.25 | 0.88+-0.25 | 6.49 |
CN | ... | <0.73 | <3.56 | <8.7 |
Mg I | ... | -2.61+-0.23 | 0.22+-0.23 | 4.99 |
Al I | ... | -3.53+-0.23 | -0.7+-0.23 | 2.92 |
Si I | ... | -2.57+-0.36 | 0.26+-0.36 | 4.94 |
Ca I | ... | -2.38+-0.23 | 0.45+-0.23 | 3.96 |
Sc II | ... | -2.49+-0.15 | 0.34+-0.15 | 0.68 |
Ti I | ... | -2.15+-0.21 | 0.68+-0.21 | 2.8 |
Ti II | ... | -2.52+-0.14 | 0.31+-0.14 | 2.44 |
V II | ... | <-1.82 | <1.01 | <2.18 |
Cr I | ... | -3.04+-0.2 | -0.21+-0.2 | 2.6 |
Mn I | ... | -3.12+-0.21 | -0.29+-0.21 | 2.31 |
Fe I | ... | -2.83+-0.22 | ... | 4.67 |
Fe II | ... | -2.81+-0.14 | ... | 4.69 |
Co I | ... | -2.48+-0.25 | 0.35+-0.25 | 2.51 |
Ni I | ... | -2.67+-0.24 | 0.16+-0.24 | 3.55 |
Sr II | ... | -2.96+-0.18 | -0.13+-0.18 | -0.08 |
Y II | ... | <-2.51 | <0.32 | <-0.27 |
Zr II | ... | <-1.91 | <0.92 | <0.69 |
Nb II | ... | <0.42 | <3.25 | <1.84 |
Tc I | ... | <1.88 | <4.71 | <1.88 |
Ba II | ... | -2.99+-0.14 | -0.16+-0.14 | -0.79 |
Ce II | ... | <-1.10 | <1.73 | <0.48 |
Pr II | ... | <-0.53 | <2.30 | <0.18 |
Nd II | ... | <-1.13 | <1.70 | <0.37 |
Sm II | ... | <-0.63 | <2.20 | <0.38 |
Eu II | ... | <-1.08 | <1.75 | <-0.57 |
Gd II | ... | <-0.53 | <2.30 | <0.59 |
Tb II | ... | <0.80 | <3.63 | <0.7 |
Dy II | ... | <-1.27 | <1.56 | <-0.13 |
Ho II | ... | <-0.19 | <2.64 | <0.07 |
Er II | ... | <-0.59 | <2.24 | <0.34 |
Tm II | ... | <-0.06 | <2.77 | <-0.06 |
Hf II | ... | <0.12 | <2.95 | <1 |
Pb I | ... | <0.10 | <2.93 | <2.05 |
Th II | ... | <0.11 | <2.94 | <0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)