Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.84-0.09 | +-0.09 | 2.1 |
CH | ... | -2.44+-0.25 | 0.4+-0.25 | 6.01 |
NH | ... | <-1.97 | <0.87 | <6 |
O I | ... | <-2.60 | <0.24 | <6.27 |
Mg I | ... | -2.47+-0.11 | 0.37+-0.11 | 5.14 |
Al I | ... | -3.61+-0.16 | -0.77+-0.16 | 2.84 |
Si I | ... | -2.16+-0.21 | 0.68+-0.21 | 5.35 |
Ca I | ... | -2.45+-0.13 | 0.39+-0.13 | 3.89 |
Sc II | ... | -2.83+-0.13 | 0.01+-0.13 | 0.33 |
Ti I | ... | -2.45+-0.11 | 0.39+-0.11 | 2.5 |
Ti II | ... | -2.51+-0.11 | 0.33+-0.11 | 2.45 |
V II | ... | -2.41+-0.29 | 0.43+-0.29 | 1.53 |
Cr I | ... | -2.99+-0.1 | -0.15+-0.1 | 2.65 |
Mn I | ... | -3.47+-0.1 | -0.63+-0.1 | 1.96 |
Mn II | ... | -3.26+-0.19 | -0.42+-0.19 | 2.18 |
Fe I | ... | -2.84+-0.1 | ... | 4.66 |
Fe II | ... | -2.83+-0.12 | ... | 4.67 |
Co I | ... | -2.56+-0.15 | 0.28+-0.15 | 2.43 |
Ni I | ... | -2.69+-0.19 | 0.15+-0.19 | 3.53 |
Zn I | ... | <-2.17 | <0.67 | <2.43 |
Rb I | ... | <-0.01 | <2.83 | <2.59 |
Sr II | ... | -2.87+-0.13 | -0.03+-0.13 | 0.01 |
Y II | ... | <-2.34 | <0.50 | <-0.1 |
Zr II | ... | <-2.14 | <0.70 | <0.46 |
Nb II | ... | <0.10 | <2.94 | <1.52 |
Mo I | ... | <-0.68 | <2.16 | <1.24 |
Tc I | ... | <1.23 | <4.07 | <1.23 |
Ba II | ... | -3.17+-0.13 | -0.33+-0.13 | -0.98 |
Ce II | ... | <-1.35 | <1.49 | <0.23 |
Pr II | ... | <-0.95 | <1.89 | <-0.24 |
Nd II | ... | <-1.25 | <1.59 | <0.25 |
Sm II | ... | <-0.98 | <1.86 | <0.03 |
Eu II | ... | <-1.73 | <1.11 | <-1.22 |
Gd II | ... | <-0.83 | <2.01 | <0.29 |
Tb II | ... | <-0.03 | <2.81 | <-0.13 |
Dy II | ... | <-1.36 | <1.48 | <-0.22 |
Er II | ... | <-0.87 | <1.97 | <0.06 |
Tm II | ... | <-0.50 | <2.34 | <-0.5 |
Yb II | ... | <-2.14 | <0.70 | <-1.06 |
Hf II | ... | <-0.15 | <2.69 | <0.73 |
Pb I | ... | <-0.15 | <2.69 | <1.8 |
Th II | ... | <-0.13 | <2.71 | <-0.13 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)