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Table 9.
Statistics of the 35 systems in this paper.
| SB | New Orb. | LPV | Inconclusive/No data | |
|---|---|---|---|---|
| 22 | 20 | 6 | 7 | |
| % | 63 | 57 | 17 | 20 |
Notes. Systems that we find not to be spectroscopic binaries are labeled as line-profile variable (LPV). It should be noted that we have included Cyg OB2-22 C in the doubtful category (see text).
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