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Table 5
Close binaries with early-type stars on the main sequence and orbital period shorter than one day (extracted from Polushina 2004).
| Name | Period (d) | Spectral type | Mass (M⊙) |
|
|
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| BH Cen | 0.792 | B3+B3 | 9.4 ± 5.4 + 7.9 ± 5.4 (1) |
| V593 Cen | 0.755 | B1 Vn | unknown |
| EM Cep | 0.806 | B0.5 V+B1 Ve | 10.51 + 9.46 (2) |
| BR Mus | 0.798 | B3 | unknown |
| V701 Sco | 0.762 | B1 V-B1.5 V | 10.3 + 10.2 (3) |
| CT Tau | 0.667 | B2+B2 | unknown |
Reference. (1) Leung et al. (1984); (2) Hohle et al. (2010); (3) Polushina (2004).
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