Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -2.08 | 0.15 | 6.47 |
NH | ... | -1.73 | 0.5 | 6.24 |
Na I | ... | -2.36+-0.1 | -0.13+-0.1 | 3.97+-0.1 |
Mg I | ... | -2.19+-0.14 | 0.04+-0.14 | 5.39+-0.14 |
Al I | ... | -2.74 | -0.51 | 3.73 |
Ca I | ... | -2.49+-0.13 | -0.26+-0.13 | 3.87+-0.13 |
Sc II | ... | -2.24+-0.14 | -0.01+-0.14 | 0.93+-0.14 |
Ti I | ... | -2.45+-0.09 | -0.22+-0.09 | 2.57+-0.09 |
Ti II | ... | -2.23+-0.13 | 0.00+-0.13 | 2.79+-0.13 |
V I | ... | -2.66 | -0.43 | 1.34 |
Cr I | ... | -2.49+-0.08 | -0.26+-0.08 | 3.18+-0.08 |
Mn I | ... | -2.34+-0.06 | -0.11+-0.06 | 3.05+-0.06 |
Fe I | ... | -2.23+-0.2 | ... | 5.27+-0.2 |
Fe II | ... | -2.15+-0.13 | 0.08+-0.13 | 5.35+-0.13 |
Co I | ... | -1.91+-0.2 | 0.32+-0.2 | 3.01+-0.2 |
Ni I | ... | -2.34+-0.24 | -0.11+-0.24 | 3.91+-0.24 |
Cu I | ... | -2.77 | -0.54 | 1.44 |
Zn I | ... | -2.54 | -0.31 | 2.06 |
Sr II | ... | -4.25 | -2.02 | -1.28 |
Ba II | ... | -3.79+-0.1 | -1.56+-0.1 | -1.66+-0.1 |
Eu II | ... | <-2.51 | <-0.28 | <-2.00 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)