Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.11-0.2 | +-0.2 | 2.2 |
CH | ... | -2.09+-0.25 | 0.02+-0.25 | 6.48 |
NH | ... | <-1.27 | <0.84 | <6.7 |
O I | ... | -1.51+-0.2 | 0.6+-0.2 | 7.18 |
Mg I | ... | -1.68+-0.24 | 0.43+-0.24 | 5.92 |
Al I | ... | -2.96+-0.33 | -0.85+-0.33 | 3.49 |
K I | ... | -1.81+-0.23 | 0.3+-0.23 | 3.22 |
Ca I | ... | -1.61+-0.23 | 0.5+-0.23 | 4.73 |
Sc II | ... | -1.98+-0.14 | 0.13+-0.14 | 1.32 |
Ti I | ... | -1.80+-0.2 | 0.31+-0.2 | 3.15 |
Ti II | ... | -1.75+-0.14 | 0.36+-0.14 | 3.34 |
V I | ... | -2.02+-0.23 | 0.09+-0.23 | 1.91 |
V II | ... | -1.86+-0.24 | 0.25+-0.24 | 2.21 |
Cr I | ... | -2.20+-0.21 | -0.09+-0.21 | 3.44 |
Cr II | ... | -1.83+-0.14 | 0.28+-0.14 | 3.95 |
Mn I | ... | -2.33+-0.22 | -0.22+-0.22 | 3.1 |
Mn II | ... | -2.55+-0.25 | -0.44+-0.25 | 3.02 |
Fe I | ... | -2.11+-0.21 | ... | 5.39 |
Fe II | ... | -1.97+-0.14 | ... | 5.53 |
Co I | ... | -2.20+-0.25 | -0.09+-0.25 | 2.78 |
Ni I | ... | -2.04+-0.28 | 0.07+-0.28 | 4.18 |
Cu I | ... | <-2.01 | <0.10 | <2.2 |
Zn I | ... | -1.82+-0.2 | 0.29+-0.2 | 2.74 |
Rb I | ... | <-0.17 | <1.94 | <2.43 |
Sr II | ... | -2.09+-0.23 | 0.02+-0.23 | 0.93 |
Y II | ... | -2.46+-0.17 | -0.35+-0.17 | -0.11 |
Zr II | ... | -1.98+-0.17 | 0.13+-0.17 | 0.75 |
Nb II | ... | <0.20 | <2.31 | <1.62 |
Mo I | ... | <-0.85 | <1.26 | <1.07 |
Tc I | ... | <1.63 | <3.74 | <1.63 |
Ba II | ... | -2.34+-0.14 | -0.23+-0.14 | -0.01 |
La II | ... | <-1.74 | <0.37 | <-0.57 |
Ce II | ... | <-1.47 | <0.64 | <0.11 |
Pr II | ... | <-0.66 | <1.45 | <0.05 |
Nd II | ... | <-1.53 | <0.58 | <-0.03 |
Sm II | ... | <-1.05 | <1.06 | <-0.04 |
Eu II | ... | -2.05+-0.22 | 0.06+-0.22 | -1.39 |
Gd II | ... | <-0.75 | <1.36 | <0.37 |
Dy II | ... | <-1.59 | <0.52 | <-0.45 |
Er II | ... | <-1.03 | <1.08 | <-0.1 |
Tm II | ... | <-0.55 | <1.56 | <-0.55 |
Hf II | ... | <-0.27 | <1.84 | <0.61 |
Pb I | ... | -0.51+-0.27 | 1.6+-0.27 | 1.53 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)