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Table 3.
Atmospheric parameters derived from optimal fitting of disentangled spectra of the components to a grid of NLTE spectra.
| Star | Teff | v sin i | ξt |
|---|---|---|---|
| (K) | (km s−1) | (km s−1) | |
| V1034 Sco A | 32 200 ± 500 | 169.8 ± 2.6 | 5 ± 1 |
| V1034 Sco B | 25 800 ± 300 | 94.5 ± 3.3 | 5 ± 1 |
| GL Car A | 30 950 ± 500 | 180.1 ± 2.2 | 4 ± 1 |
| GL Car B | 30 400 ± 500 | 134.6 ± 3.5 | 2 ± 1 |
| V573 Car A | 31 900 ± 400 | 184.6 ± 2.7 | 5 ± 1 |
| V573 Car B | 28 700 ± 350 | 155.4 ± 3.1 | 3 ± 1 |
| V346 Cen A | 26 100 ± 300 | 165.2 ± 2.8 | 5 ± 1 |
| V346 Cen B | 22 500 ± 300 | 89.1 ± 2.3 | 5 ± 1 |
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