Table 4
Mass transfer and mass loss through stellar wind rates for our selected stars.
| Star | Used Ṗ |  mass transfer |
stellar wind |
| value | (10-6M⊙ yr-1) | (10-6M⊙ yr-1) | |
| A36 | Ṗ emp | 48 ± 19 | 56 ± 19 |
| Ṗ model | 50 ± 21 | -58 ± 19 | |
| MT059 | Ṗ emp | -10.5 ± 4 | − |
| Ṗ model | -8.0 ± 3 | − | |
| MT696 | Ṗ emp | -41 ± 160 | − |
| Ṗ model | -50 ± 254 | − | |
| MT720 | Ṗ emp | 104 ± 30 | -10.7 ± 4.2 |
| Ṗ model | -149 ± 45 | − | |
| Schulte 3 | Ṗ emp | -13.9 ± 10.2 | − |
| Ṗ model | 0.001 ± 8.8 | − | |
| Schulte 5 | Ṗ emp | 3.0 ± 0.2 | -15.6 ± 0.7 |
| Ṗ model | 3.4 ± 0.2 | −17.4 ± 0.8 | |
Notes. No mass loss through stellar wind is given for the negative Ṗ value as this would indicate a positive mass loss from the primary. The errors are calculated using the P, Ṗ, M1, and M2 uncertainties. The errors for MT696 are large as a result of the similar companion masses. The two period change values (Ṗemp and Ṗmodel) for each star are given in Table 2. B17 is omitted from the table as there are no mass estimates.
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