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Table 2.
Values for qcrit used in the simulations.
| Evolutionary state of donor | qcrit value for each qset | ||||
|---|---|---|---|---|---|
| 1 | 2 | 3 | 4 | 5 | |
| MS, < 0.7 M⊙ | 0.695 | 0.695 | 0.695 | 0.695 | 0.695 |
| MS, > 0.7 M⊙ | 1.6 | 1.6 | 1.6 | 1.6 | 1.6 |
| Hertzsprung gap | 4.0 | 4.0 | 4.0 | 4.0 | 4.0 |
| First ascent giant branch (FGB) | Eq. (1) | Eq. (1) | 2.0 | Eq. (1) | 2.0 |
| Core helium burning | 3.0 | 3.0 | 3.0 | 3.0 | 3.0 |
| Early asymptotic giant branch (AGB) | Eq. (1) | 2.0 | Eq. (1) | Eq. (1) | 2.0 |
| Thermally pulsing AGB (TAGB) | Eq. (1) | Eq. (1) | Eq. (1) | 2.0 | 2.0 |
Notes. Each qset (from 1 to 4) has a defined value for qcrit, the critical mass ratio for the onset of unstable mass transfer (Mdonor/Maccretor), depending on the evolutionary state of the donor star. Eq. (1) from Claeys et al. (2014).
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