Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.02-0.21 | +-0.21 | 1.88 |
CH | ... | <-2.20 | <0.82 | <6.35 |
NH | ... | <-1.32 | <1.70 | <6.65 |
O I | ... | -2.76+-0.22 | 0.26+-0.22 | 5.92 |
Mg I | ... | -2.56+-0.21 | 0.46+-0.21 | 5.04 |
Al I | ... | -3.66+-0.22 | -0.64+-0.22 | 2.78 |
Si I | ... | -2.66+-0.36 | 0.36+-0.36 | 4.85 |
Ca I | ... | -2.43+-0.22 | 0.59+-0.22 | 3.91 |
Sc II | ... | -2.92+-0.15 | 0.1+-0.15 | 0.4 |
Ti I | ... | -2.33+-0.21 | 0.69+-0.21 | 2.61 |
Ti II | ... | -2.69+-0.14 | 0.33+-0.14 | 2.42 |
V II | ... | <-2.04 | <0.98 | <1.96 |
Cr I | ... | -3.24+-0.2 | -0.22+-0.2 | 2.39 |
Cr II | ... | -2.56+-0.16 | 0.46+-0.16 | 3.25 |
Mn I | ... | -3.41+-0.22 | -0.39+-0.22 | 2.01 |
Mn II | ... | -3.40+-0.2 | -0.38+-0.2 | 2.19 |
Fe I | ... | -3.02+-0.21 | ... | 4.48 |
Fe II | ... | -2.85+-0.15 | ... | 4.65 |
Co I | ... | -2.77+-0.24 | 0.25+-0.24 | 2.22 |
Ni I | ... | -3.04+-0.26 | -0.02+-0.26 | 3.18 |
Zn I | ... | <-2.07 | <0.95 | <2.53 |
Rb I | ... | <0.37 | <3.39 | <2.97 |
Sr II | ... | -3.11+-0.19 | -0.09+-0.19 | -0.07 |
Y II | ... | -3.36+-0.4 | -0.34+-0.4 | -0.98 |
Nb II | ... | <0.15 | <3.17 | <1.57 |
Mo I | ... | <-0.43 | <2.59 | <1.49 |
Tc I | ... | <1.71 | <4.73 | <1.71 |
Sn I | ... | <0.53 | <3.55 | <2.53 |
Ba II | ... | -3.73+-0.15 | -0.71+-0.15 | -1.38 |
Ce II | ... | <-1.34 | <1.68 | <0.24 |
Pr II | ... | <-0.88 | <2.14 | <-0.17 |
Nd II | ... | <-1.31 | <1.71 | <0.19 |
Sm II | ... | <-0.81 | <2.21 | <0.2 |
Eu II | ... | <-1.68 | <1.34 | <-1.17 |
Gd II | ... | <-0.64 | <2.38 | <0.48 |
Tb II | ... | <-0.01 | <3.01 | <-0.11 |
Dy II | ... | <-1.18 | <1.84 | <-0.04 |
Er II | ... | <-0.96 | <2.06 | <-0.03 |
Tm II | ... | <-0.46 | <2.56 | <-0.46 |
Yb II | ... | <-2.10 | <0.92 | <-1.02 |
Hf II | ... | <-0.12 | <2.90 | <0.76 |
Pb I | ... | <-0.12 | <2.90 | <1.83 |
Th II | ... | <-0.06 | <2.96 | <-0.06 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)