Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.00-0.2 | +-0.2 | 2.04 |
CH | ... | -2.66+-0.25 | 0.34+-0.25 | 5.91 |
NH | ... | <-1.97 | <1.03 | <6 |
O I | ... | <-2.37 | <0.63 | <6.5 |
Mg I | ... | -2.55+-0.22 | 0.45+-0.22 | 5.04 |
Al I | ... | -3.69+-0.28 | -0.69+-0.28 | 2.76 |
Si I | ... | -2.40+-0.36 | 0.6+-0.36 | 5.11 |
K I | ... | -2.57+-0.25 | 0.43+-0.25 | 2.46 |
Ca I | ... | -2.52+-0.22 | 0.48+-0.22 | 3.82 |
Sc II | ... | -3.16+-0.16 | -0.16+-0.16 | 0.12 |
Ti I | ... | -2.73+-0.21 | 0.27+-0.21 | 2.22 |
Ti II | ... | -2.87+-0.13 | 0.13+-0.13 | 2.22 |
Cr I | ... | -3.28+-0.2 | -0.28+-0.2 | 2.36 |
Mn I | ... | -3.43+-0.2 | -0.43+-0.2 | 2 |
Mn II | ... | -3.54+-0.21 | -0.54+-0.21 | 2.03 |
Fe I | ... | -3+-0.22 | ... | 4.5 |
Fe II | ... | -2.86+-0.14 | ... | 4.64 |
Co I | ... | -2.82+-0.24 | 0.18+-0.24 | 2.17 |
Ni I | ... | -3.07+-0.27 | -0.07+-0.27 | 3.15 |
Zn I | ... | <-2.19 | <0.81 | <2.41 |
Rb I | ... | <0.06 | <3.06 | <2.66 |
Sr II | ... | -3.26+-0.19 | -0.26+-0.19 | -0.25 |
Y II | ... | <-2.93 | <0.07 | <-0.69 |
Zr II | ... | <-2.35 | <0.65 | <0.25 |
Nb II | ... | <0.03 | <3.03 | <1.45 |
Mo I | ... | <-0.91 | <2.09 | <1.01 |
Tc I | ... | <1.39 | <4.39 | <1.39 |
Ba II | ... | -3.71+-0.14 | -0.71+-0.14 | -1.39 |
La II | ... | <-1.92 | <1.08 | <-0.75 |
Ce II | ... | <-1.72 | <1.28 | <-0.14 |
Pr II | ... | <-1.08 | <1.92 | <-0.37 |
Nd II | ... | <-1.71 | <1.29 | <-0.21 |
Sm II | ... | <-1.05 | <1.95 | <-0.04 |
Eu II | ... | <-1.92 | <1.08 | <-1.41 |
Gd II | ... | <-0.85 | <2.15 | <0.27 |
Tb II | ... | <-0.30 | <2.70 | <-0.4 |
Dy II | ... | <-1.59 | <1.41 | <-0.45 |
Ho II | ... | <-0.76 | <2.24 | <-0.5 |
Er II | ... | <-1.28 | <1.72 | <-0.35 |
Tm II | ... | <-0.64 | <2.36 | <-0.64 |
Yb II | ... | <-2.34 | <0.66 | <-1.26 |
Hf II | ... | <-0.27 | <2.73 | <0.61 |
Pb I | ... | <-0.50 | <2.50 | <1.45 |
Th II | ... | <-0.33 | <2.67 | <-0.33 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)