Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.20-0.2 | +-0.2 | 2.25 |
CH | ... | <-1.50 | <0.70 | <7.05 |
CN | ... | <0.23 | <2.43 | <8.2 |
Mg I | ... | -1.70+-0.22 | 0.5+-0.22 | 5.9 |
Al I | ... | -2.80+-0.34 | -0.6+-0.34 | 3.65 |
Si I | ... | -1.83+-0.38 | 0.37+-0.38 | 5.68 |
Ca I | ... | -1.74+-0.22 | 0.46+-0.22 | 4.61 |
Sc II | ... | -2.15+-0.18 | 0.05+-0.18 | 1.14 |
Ti I | ... | -1.55+-0.2 | 0.65+-0.2 | 3.4 |
Ti II | ... | -1.73+-0.18 | 0.47+-0.18 | 3.35 |
V II | ... | <-1.63 | <0.57 | <2.37 |
Cr I | ... | -2.35+-0.21 | -0.15+-0.21 | 3.3 |
Mn I | ... | -2.49+-0.2 | -0.29+-0.2 | 2.94 |
Fe I | ... | -2.2+-0.21 | ... | 5.3 |
Fe II | ... | -2.06+-0.18 | ... | 5.44 |
Co I | ... | -2.05+-0.22 | 0.15+-0.22 | 2.94 |
Cu I | ... | <-1.30 | <0.90 | <2.91 |
Zn I | ... | <-1.58 | <0.62 | <3.02 |
Sr II | ... | -1.66+-0.24 | 0.54+-0.24 | 1.35 |
Y II | ... | <-1.65 | <0.55 | <0.59 |
Zr II | ... | <-1.43 | <0.77 | <1.17 |
Nb II | ... | <0.67 | <2.87 | <2.09 |
Mo I | ... | <0.15 | <2.35 | <2.07 |
Tc I | ... | <2.06 | <4.26 | <2.06 |
Ba II | ... | -2.48+-0.19 | -0.28+-0.19 | -0.16 |
Ce II | ... | <-0.97 | <1.23 | <0.61 |
Pr II | ... | <-0.40 | <1.80 | <0.31 |
Nd II | ... | <-0.95 | <1.25 | <0.55 |
Sm II | ... | <-0.52 | <1.68 | <0.49 |
Eu II | ... | <-1.16 | <1.04 | <-0.65 |
Gd II | ... | <-0.21 | <1.99 | <0.91 |
Tb II | ... | <0.71 | <2.91 | <0.61 |
Dy II | ... | <-0.80 | <1.40 | <0.34 |
Er II | ... | <-0.38 | <1.82 | <0.55 |
Tm II | ... | <0.25 | <2.45 | <0.25 |
Hf II | ... | <0.26 | <2.46 | <1.14 |
Pb I | ... | <0.36 | <2.56 | <2.31 |
Th II | ... | <0.41 | <2.61 | <0.41 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)