Table 1
Atomic parameters of the observed lines.
| Ion | λ0 (Å) | χl | log (gf) | Elec. configurations | σ | α |
|
|
|
|||||||
| Fe i | 15 648.515 | 5.426 | –0.739 |
|
975 | 0.229 | 3.00 |
| Fe i | 15 652.874 | 6.246 | –0.165 |
|
1427 | 0.330 | 1.45 |
| Fe i | 15 662.018 | 5.828 | 0.120 |
|
1200 | 0.24 | 1.50 |
| Fe i | 15 665.245 | 5.979 | –0.490 |
|
1283 | 0.23 | 0.75 |
| Fe i | 6173.336 | 2.223 | –2.919 |
|
281 | 0.27 | 2.50 |
Notes. The first column indicates the ion, λ0 is the laboratory wavelength, χl is the excitation potential of the lower energy level in eV, log (gf) is the logarithm of the oscillator strength multiplied by the multiplicity of the level, σ (in units of the Bohr radius squared, 
) and α are the collisional broadening parameters, and is the effective Landé factor. The tabulated values of log (gf) correspond to a solar iron abundance of 7.50 dex (Asplund et al. 2009).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.