Table B.2.
Tabulation of our main results.
| ZAMS mass | model | log(R) | mass|RLOF | log(ṀKH) | log(Ṁth,crit) | qqad | qOLOF | qdyn |
|---|---|---|---|---|---|---|---|---|
| M⊙ | – | R⊙ | M⊙ | M⊙ yr−1 | M⊙ yr−1 | Ma/Md | Ma/Md | Ma/Md |
| 1.0 | 0 | 0.129 | 0.9995 | -6.820 | -3.990 | 0.431 ± 0.006 | † | † |
| 1.0 | 1 | 0.252 | 0.9994 | -6.600 | -3.860 | 0.744 ± 0.006 | † | † |
| 1.0 | 2 | 0.447 | 0.9993 | -6.163 | -3.590 | 1.031 ± 0.006 | † | † |
| 1.0 | 3 | 0.645 | 0.9991 | -5.607 | -3.217 | 1.006 ± 0.006 | † | † |
| 1.0 | 4 | 0.841 | 0.9988 | -5.073 | -2.865 | 0.956 ± 0.006 | † | † |
Notes. This table shows the critical mass ratios corresponding to the criteria described in Sect. 3. For qdyn, Adyn = 0.05 was assumed. For mass ratios smaller than the tabulated values, mass transfer is unstable according to the related criterion. A dagger symbol (†) indicates where the mass transfer became unstable and our simulations ended before reaching either the dynamical-timescale or OLOF criteria. Additionally, this table enumerates, for each single star model used as starting point for the donor star in our binary calculations, the critical mass-transfer rate and the KH mass-transfer rate (as defined in Sect. 3.3). For brevity, only the first five rows are shown here. The full is available on request or in electronic form at the CDS via anonymous ftp to cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/vol/page
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