Table 4.
Estimated masses of the unseen secondaries of the five SB1s.
| ID | mspec, l | mspec, u | mevo, l | mevo, u | mlim, MS | mlim, strip | imin |
|---|---|---|---|---|---|---|---|
| M⊙ | M⊙ | M⊙ | M⊙ | M⊙ | M⊙ | ° | |
| HD 152200 | 1.3 | 3.5 | 1.1 | 2.6 | 2.2 | 2 | 23±8 |
| V* V946 Sco | 2.7 | 7.8 | 2.5 | 7.2 | 1.4 | 1 | 25±7 |
| CD−41 11038 | 2.4 | 26 | 1.6 | 13.7 | 2.2 | 2 | 7.5±0.9 |
| CXOU J165421.3-415536 | 0.9 | 3.1 | 0.9 | 3.1 | 1.4 | 1 | 20±3 |
| CPD−41 7717 | 0.4 | 0.9 | 0.5 | 1.2 | 1.4 | 1 | 29±8 |
Notes. mspec, l and mspec, u are the lower and upper companion mass estimates respectively, based on the spectroscopic estimate of the primary mass. mevo, l and mevo, u are the same based on the evolutionary estimate of the primary mass. Also included are the lower detection limits of the spectral disentangling for main sequence (mlim, MS) and stripped (mlim, strip) stars, and the minimum estimated inclination (imin) of each system.
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