Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.84 | <3.99 | <2 |
CH | ... | <-1.60 | <1.55 | <6.95 |
NH | ... | <-0.72 | <2.43 | <7.25 |
O I | ... | -2.76+-0.17 | 0.39+-0.17 | 5.93 |
Na I | ... | -3.24+-0.19 | -0.09+-0.19 | 3 |
Mg I | ... | -2.86+-0.19 | 0.29+-0.19 | 4.74 |
Al I | ... | -3.90+-0.18 | -0.75+-0.18 | 2.55 |
Si I | ... | -3.15+-0.24 | 0.00+-0.24 | 4.36 |
Ca I | ... | -2.76+-0.2 | 0.39+-0.2 | 3.58 |
Sc II | ... | -3.11+-0.15 | 0.04+-0.15 | 0.05 |
Ti II | ... | -2.96+-0.15 | 0.19+-0.15 | 2 |
Cr I | ... | -3.20+-0.16 | -0.05+-0.16 | 2.45 |
Mn I | ... | -3.55+-0.18 | -0.4+-0.18 | 1.88 |
Mn II | ... | -3.25+-0.21 | -0.1+-0.21 | 2.18 |
Fe I | ... | -3.15+-0.17 | ... | 4.35 |
Fe II | ... | -3.14+-0.16 | ... | 4.36 |
Ni I | ... | -3.05+-0.21 | 0.1+-0.21 | 3.17 |
Zn I | ... | <-2.07 | <1.08 | <2.53 |
Sr II | ... | -2.89+-0.24 | 0.26+-0.24 | -0.02 |
Y II | ... | <-2.69 | <0.46 | <-0.45 |
Zr II | ... | <-2.58 | <0.57 | <0.02 |
Nb II | ... | <-0.36 | <2.79 | <1.06 |
Mo I | ... | <-0.52 | <2.63 | <1.4 |
Tc I | ... | <1.76 | <4.91 | <1.76 |
Ba II | ... | -4.32+-0.16 | -1.17+-0.16 | -2.13 |
Ce II | ... | <-1.84 | <1.31 | <-0.26 |
Pr II | ... | <-1.22 | <1.93 | <-0.51 |
Nd II | ... | <-1.85 | <1.30 | <-0.35 |
Sm II | ... | <-1.31 | <1.84 | <-0.3 |
Eu II | ... | <-2.05 | <1.10 | <-1.54 |
Gd II | ... | <-1.14 | <2.01 | <-0.02 |
Tb II | ... | <-0.43 | <2.72 | <-0.53 |
Dy II | ... | <-1.84 | <1.31 | <-0.7 |
Er II | ... | <-1.34 | <1.81 | <-0.41 |
Tm II | ... | <-0.89 | <2.26 | <-0.89 |
Hf II | ... | <-0.70 | <2.45 | <0.18 |
Pb I | ... | <-0.02 | <3.13 | <1.93 |
Th II | ... | <-0.57 | <2.58 | <-0.57 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)