Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.05-0.2 | +-0.2 | 1.99 |
CH | ... | -2.87+-0.25 | 0.18+-0.25 | 5.83 |
NH | ... | <-2.17 | <0.88 | <5.8 |
O I | ... | <-2.46 | <0.59 | <6.41 |
Mg I | ... | -2.62+-0.22 | 0.43+-0.22 | 4.98 |
Al I | ... | -3.81+-0.23 | -0.76+-0.23 | 2.64 |
Si I | ... | -2.74+-0.36 | 0.31+-0.36 | 4.77 |
Ca I | ... | -2.58+-0.22 | 0.47+-0.22 | 3.76 |
Sc II | ... | -3.21+-0.16 | -0.16+-0.16 | 0.22 |
Ti I | ... | -2.62+-0.21 | 0.43+-0.21 | 2.33 |
Ti II | ... | -2.87+-0.14 | 0.18+-0.14 | 2.35 |
Cr I | ... | -3.32+-0.21 | -0.27+-0.21 | 2.32 |
Cr II | ... | -2.94+-0.24 | 0.11+-0.24 | 2.98 |
Mn I | ... | -3.54+-0.2 | -0.49+-0.2 | 1.89 |
Mn II | ... | -3.47+-0.2 | -0.42+-0.2 | 2.24 |
Fe I | ... | -3.05+-0.22 | ... | 4.45 |
Fe II | ... | -2.77+-0.15 | ... | 4.73 |
Co I | ... | -2.89+-0.24 | 0.16+-0.24 | 2.1 |
Ni I | ... | -3.06+-0.26 | -0.01+-0.26 | 3.16 |
Zn I | ... | <-2.27 | <0.78 | <2.33 |
Sr II | ... | -3.78+-0.15 | -0.73+-0.15 | -0.63 |
Y II | ... | <-2.44 | <0.61 | <-0.2 |
Zr II | ... | <-2.42 | <0.63 | <0.18 |
Nb II | ... | <0.00 | <3.05 | <1.42 |
Mo I | ... | <-0.92 | <2.13 | <1 |
Ba II | ... | <-3.84 | <-0.79 | <-1.71 |
La II | ... | <-1.97 | <1.08 | <-0.8 |
Ce II | ... | <-1.56 | <1.49 | <0.02 |
Pr II | ... | <-1.10 | <1.95 | <-0.39 |
Nd II | ... | <-1.63 | <1.42 | <-0.13 |
Sm II | ... | <-1.09 | <1.96 | <-0.08 |
Eu II | ... | <-1.86 | <1.19 | <-1.35 |
Gd II | ... | <-0.89 | <2.16 | <0.23 |
Tb II | ... | <-0.28 | <2.77 | <-0.38 |
Dy II | ... | <-1.58 | <1.47 | <-0.44 |
Ho II | ... | <-0.89 | <2.16 | <-0.63 |
Er II | ... | <-1.08 | <1.97 | <-0.15 |
Tm II | ... | <-0.52 | <2.53 | <-0.52 |
Yb II | ... | <-2.30 | <0.75 | <-1.22 |
Hf II | ... | <-0.34 | <2.71 | <0.54 |
Pb I | ... | <-0.34 | <2.71 | <1.61 |
Th II | ... | <-0.29 | <2.76 | <-0.29 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)