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Table A.3.
Spectral lines and their respective wavelength ranges, which were fitted against the FASTWIND atmosphere modeling in Sect. 4, for the primary and secondary star.
| Spectral line | λmin[Å] | λmax[Å] |
|---|---|---|
| He I 4026 | 4022.0 | 4029.8 |
| N IV 4058 | 4056.5 | 4059.9 |
| Hδ | 4093.6 | 4107.9 |
| He II 4200 | 4195.5 | 4204.3 |
| Hγ | 4332.5 | 4348.4 |
| He I 4471 | 4468.6 | 4474.0 |
| He II 4541 | 4535.5 | 4547.3 |
| N V 4604 | 4600.3 | 4608.5 |
| N V 4619 | 4617.4 | 4622.8 |
| He II 4686 | 4680.6 | 4690.4 |
| Hβ | 4850.8 | 4870.9 |
| He II 5411 | 5405.4 | 5417.1 |
| O III 5592 | 5589.3 | 5595.4 |
| C III 5696 | 5692.4 | 5698.8 |
| C IV 5801 | 5798.8 | 5805.0 |
| C IV 5812 | 5809.3 | 5815.0 |
| He I 5875 | 5872.0 | 5878.9 |
| Hα | 6551.7 | 6571.2 |
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