Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.10-0.2 | +-0.2 | 2.02 |
CH | ... | <-2.15 | <0.95 | <6.4 |
CN | ... | <-0.47 | <2.63 | <7.5 |
Mg I | ... | -2.68+-0.24 | 0.42+-0.24 | 4.91 |
Al I | ... | -3.78+-0.22 | -0.68+-0.22 | 2.66 |
Si I | ... | -2.71+-0.36 | 0.39+-0.36 | 4.8 |
Ca I | ... | -2.59+-0.23 | 0.51+-0.23 | 3.74 |
Sc II | ... | -3.21+-0.14 | -0.11+-0.14 | 0.16 |
Ti II | ... | -2.99+-0.14 | 0.11+-0.14 | 2.17 |
Cr I | ... | -3.35+-0.2 | -0.25+-0.2 | 2.29 |
Mn I | ... | -3.59+-0.2 | -0.49+-0.2 | 1.84 |
Fe I | ... | -3.1+-0.21 | ... | 4.4 |
Fe II | ... | -2.88+-0.15 | ... | 4.62 |
Co I | ... | -2.72+-0.23 | 0.38+-0.23 | 2.27 |
Cu I | ... | <-1.65 | <1.45 | <2.56 |
Ga I | ... | <-1.01 | <2.09 | <1.87 |
Sr II | ... | -3.48+-0.17 | -0.38+-0.17 | -0.39 |
Y II | ... | <-2.03 | <1.07 | <0.21 |
Zr II | ... | <-2.16 | <0.94 | <0.44 |
Nb II | ... | <0.54 | <3.64 | <1.96 |
Mo I | ... | <-0.45 | <2.65 | <1.47 |
Tc I | ... | <1.80 | <4.90 | <1.8 |
Ba II | ... | -4.24+-0.18 | -1.14+-0.18 | -1.84 |
Ce II | ... | <-1.27 | <1.83 | <0.31 |
Pr II | ... | <-0.90 | <2.20 | <-0.19 |
Nd II | ... | <-1.33 | <1.77 | <0.17 |
Sm II | ... | <-0.85 | <2.25 | <0.16 |
Eu II | ... | <-1.61 | <1.49 | <-1.1 |
Gd II | ... | <-0.53 | <2.57 | <0.59 |
Tb II | ... | <0.04 | <3.14 | <-0.06 |
Dy II | ... | <-1.33 | <1.77 | <-0.19 |
Er II | ... | <-0.62 | <2.48 | <0.31 |
Tm II | ... | <-0.32 | <2.78 | <-0.32 |
Hf II | ... | <-0.12 | <2.98 | <0.76 |
Pb I | ... | <-0.09 | <3.01 | <1.86 |
Th II | ... | <-0.02 | <3.08 | <-0.02 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)