Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.69-0.2 | +-0.2 | 2.26 |
CH | ... | <-1.55 | <1.14 | <7 |
NH | ... | <-0.77 | <1.92 | <7.2 |
O I | ... | -2.73+-0.21 | -0.04+-0.21 | 5.96 |
Mg I | ... | -2.33+-0.22 | 0.36+-0.22 | 5.27 |
Al I | ... | -3.35+-0.25 | -0.66+-0.25 | 3.1 |
Si I | ... | -2.26+-0.36 | 0.43+-0.36 | 5.25 |
K I | ... | -2.32+-0.26 | 0.37+-0.26 | 2.71 |
Ca I | ... | -2.17+-0.22 | 0.52+-0.22 | 4.17 |
Sc II | ... | -2.48+-0.15 | 0.21+-0.15 | 0.76 |
Ti II | ... | -2.28+-0.14 | 0.41+-0.14 | 2.76 |
V II | ... | -1.97+-0.27 | 0.72+-0.27 | 2.05 |
Cr I | ... | -2.68+-0.2 | 0.01+-0.2 | 2.96 |
Cr II | ... | -2.40+-0.16 | 0.29+-0.16 | 3.33 |
Mn I | ... | -2.86+-0.21 | -0.17+-0.21 | 2.57 |
Mn II | ... | -3.09+-0.21 | -0.4+-0.21 | 2.43 |
Fe I | ... | -2.69+-0.22 | ... | 4.81 |
Fe II | ... | -2.6+-0.15 | ... | 4.9 |
Co I | ... | -2.46+-0.24 | 0.23+-0.24 | 2.53 |
Ni I | ... | -2.58+-0.26 | 0.11+-0.26 | 3.64 |
Zn I | ... | <-1.89 | <0.80 | <2.71 |
Rb I | ... | <0.21 | <2.90 | <2.81 |
Sr II | ... | -2.66+-0.22 | 0.03+-0.22 | 0.3 |
Zr II | ... | <-1.37 | <1.32 | <1.23 |
Nb II | ... | <0.55 | <3.24 | <1.97 |
Mo I | ... | <-0.22 | <2.47 | <1.7 |
Tc I | ... | <2.10 | <4.79 | <2.1 |
Ba II | ... | -3.19+-0.14 | -0.5+-0.14 | -0.92 |
La II | ... | <-1.39 | <1.30 | <-0.22 |
Ce II | ... | <-0.92 | <1.77 | <0.66 |
Pr II | ... | <-0.54 | <2.15 | <0.17 |
Nd II | ... | <-1.10 | <1.59 | <0.4 |
Sm II | ... | <-0.47 | <2.22 | <0.54 |
Eu II | ... | <-1.26 | <1.43 | <-0.75 |
Gd II | ... | <-0.42 | <2.27 | <0.7 |
Tb II | ... | <0.44 | <3.13 | <0.34 |
Dy II | ... | <-1.00 | <1.69 | <0.14 |
Ho II | ... | <-0.14 | <2.55 | <0.12 |
Er II | ... | <-0.53 | <2.16 | <0.4 |
Tm II | ... | <1.07 | <3.76 | <1.07 |
Yb II | ... | <-1.70 | <0.99 | <-0.62 |
Hf II | ... | <0.36 | <3.05 | <1.24 |
Pb I | ... | <0.18 | <2.87 | <2.13 |
Th II | ... | <0.23 | <2.92 | <0.23 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)