Table 8.
Results of the MONOS II analysis for systems where we do not find the O star to show a spectroscopic orbital motion.
| Name | SBS classification |
VRx−corr | VRHe ii λ5412 | VRO iii λ5592 | v sin i | Notes | |
|---|---|---|---|---|---|---|---|
| MONOS I | MONOS II | km s−1 | km s−1 | km s−1 | km s−1 | ||
| 9 Sge | SB1? | Single | 16.9(53) | 20.3(52) | 23.7(47) | 69(3) | LPV |
| HD 192 281 | SB1 | Single | −28.8(49) | −26.0(42) | −6.0(57) | 277(14) | LPV |
| HDE 229 232 AB | SB1+Ca? | Single | −20.7(59) | −16.6(113) | ... | 313(16) | LPV |
| Cyg OB2-22 C | SB1E? | SB1 unc.+E | ... | 31.0(46) | ... | 266(14) | Triple system |
| 68 Cyg | SB1? | Single | 30.1(106) | 49.3(84) | 43.5(208) | 312(16) | LPV |
| HD 108 | SB1? | Single | ... | −75.5(47) | −71.3(43) | 46(2) | LPV |
| α Cam | SB1? | Single | 15.0(77) | 20.7(46) | 22.7(54) | 113(6) | LPV |
Notes.
LPV (line-profile variable) indicates that we were unable to determine the origin of the line variation. The RVs of the objects are obtained as described in Sect. 2.1.2. Errors are in parentheses, corresponding to the last digits.
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