Table 3
Atmospheric abundances for 43 Cygni with the error estimates based on the internal scattering from the number of the analysed lines compared to solar values.
| Element | 43 Cyg | Sun |
| log(Nel/Ntot) | log(Nel/Ntot) | |
|
|
||
| C | –3.59 ± 0.36 | –3.52 |
| O | –3.23 ± 0.07 | –3.21 |
| Na | –5.48 ± 0.04 | –5.71 |
| Mg | –4.39 ± 0.14 | –4.46 |
| Si | –4.38 ± 0.25 | –4.49 |
| Ca | –5.63 ± 0.08 | –5.68 |
| Sc | –8.73 ± 0.09 | –8.87 |
| Ti | –7.02 ± 0.10 | –7.02 |
| Cr | –6.40 ± 0.29 | –6.37 |
| Mn | –6.87 ± 0.23 | –6.65 |
| Fe | –4.56 ± 0.08 | –4.54 |
| Ni | –5.78 ± 0.28 | –5.79 |
| Cu | –7.84 ± 0.22 | –7.83 |
| Y | –9.81 ± 0.14 | –9.80 |
| Ba | –9.73 ± 0.08 | –9.91 |
Notes. Abundances of O, Na, Ca, and Ba were calculated in non-LTE based on Piskunov et al. (2017), all other elements in LTE. For comparison, the last column gives the abundances of the solar atmosphere calculated by Asplund et al. (2009).
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