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Table 2.

Properties of our detailed binary models.

max log / Outcome Outcome Outcome Outcome
# M1i/ M M2i/ M Pi/ d Case M/yr det. model with max() with Eq. (9) of Sect. 3.2
1 10 4 1.8 A −3.22 Stable, L2O Stable, L2O Stable, stripping L2O
2 10 4 10 Br −2.92 Unstable, L2O Unstable, L2O Unstable, L2O L2O
3 10 4 56 Br −2.71 Unstable, L2O Unstable, L2O Unstable, L2O L2O
4 10 4 316 Bc No solution Unstable, L2O Unstable, L2O L2O
5 10 6 1.8 A −3.82 Stable, stripping Stable, stripping Stable, stripping Stripping
6 10 6 10 Br −3.04 Stable, stripping Stable, stripping Stable, stripping Stripping
7 10 6 56 Br −2.75 Stable, L2O Stable, contact Unstable, L2O L2O
8 10 6 316 Bc No solution Unstable, L2O Unstable, L2O L2O
9 10 8 1.8 A −4.30 Stable, stripping Stable, stripping Stable, stripping Stripping
10 10 8 10 Br −3.07 Stable, stripping Stable, stripping Stable, stripping Stripping
11 10 8 56 Br −2.75 Stable, stripping Stable, stripping Stable, stripping L2O
12 10 8 316 Bc No solution Unstable, L2O Unstable, L2O L2O
13 30 12 1.8 A −2.42 Unstable, L2O Stable, L2O Stable, stripping Stripping
14 30 12 10 Br −1.96 Unstable, L2O Unstable, L2O Unstable, L2O L2O
15 30 12 56 Br −2.24 Unstable, L2O Unstable, L2O Unstable, L2O L2O
16 30 12 316 Br −2.18 Unstable, L2O Unstable, L2O Unstable, L2O L2O

Notes. Initial masses M1i and M2i and initial orbital periods Pi of our detailed binary models and the case of RLO through which they pass. We distinguish between Case B with a donor with a radiative (Br) and a convective (Bc) envelope. The maximum mass-transfer rates of the detailed binary models (ε = 50%) are given as well. We display the outcomes of the RLO according to the detailed binary models (Sect.2.3.2), the radius estimate using the maximum mass-transfer rate of the detailed binary models (the crosses in Fig. 6), the radius estimate based on Eq. (9) (the plusses in Fig. 6), and the outcome from Sect. 3.2. We qualify the stability of the swelling and the occurrence of L2 overflow (L2O), contact, or neither (donor stripping).

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