Table 5.
Estimated primary (M1) and secondary masses (M2), semi-major axes (a) (units are M⊙ and R⊙), and fractional stellar radii (r) for the primaries in the SB1 sample that appear to be synchronised.
| VFTS | P (d) | M1 | M2 | a | r | RL | fL |
|---|---|---|---|---|---|---|---|
| 009 | 4.71 | 12.0 | 2.5 | 28.8 | 0.26 | 14.3 | 0.52 |
| 027 | 6.58 | 12.2 | 6.7 | 39.3 | 0.41 | 17.0 | 0.95 |
| 033 | 3.86 | 10.4 | 1.8 | 23.8 | 0.30 | 12.4 | 0.58 |
| 179 | 1.16 | 10.6 | 1.7 | 10.7 | 0.47 | 5.1 | 0.97 |
| 189 | 1.43 | 13.0 | 3.4 | 13.6 | 0.49 | 6.5 | 1.02 |
| 225 | 8.24 | 12.8 | 1.9 | 42.1 | 0.25 | 22.3 | 0.47 |
| 246 | 2.44 | 12.2 | 2.8 | 18.8 | 0.53 | 9.6 | 1.04 |
| 305 | 4.18 | 8.8 | 2.1 | 24.2 | 0.19 | 12.0 | 0.38 |
| 324 | 1.64 | 13.0 | 3.7 | 15.0 | 0.43 | 7.1 | 0.91 |
| 342 | 4.28 | 7.8 | 1.4 | 23.2 | 0.19 | 11.2 | 0.39 |
| 434 | 5.61 | 10.6 | 2.2 | 31.0 | 0.28 | 15.2 | 0.58 |
| 534 | 3.69 | 17.0 | 6.3 | 28.3 | 0.37 | 12.7 | 0.82 |
| 662 | 1.99 | 7.2 | 0.6 | 13.2 | 0.68 | 7.8 | 1.15 |
| 705 | 2.26 | 11.0 | 5.2 | 18.3 | 0.34 | 7.8 | 0.80 |
| 730 | 1.33 | 12.0 | 0.3 | 11.7 | 0.65 | 8.0 | 0.96 |
| 788 | 3.26 | 10.6 | 3.3 | 22.2 | 0.34 | 10.7 | 0.71 |
| 888 | 1.97 | 11.0 | 3.8 | 16.2 | 0.34 | 7.7 | 0.71 |
| 891 | 5.48 | 9.2 | 0.6 | 28.0 | 0.23 | 12.5 | 0.52 |
Notes. Also listed are their estimated primary Roche lobe radii (RL in R⊙) and the ratios to the stellar radii to their Roche lobe radii (fL).
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