Table 2: Non-rotating WR+O progenitor models for $\beta =0.1$. N is the number of the model, $M_{\rm 1,in}$ and $M_{\rm 2,in}$ are initial masses of the primary and the secondary, $p_{\rm in}$ is the initial orbital period and  $q_{\rm in}$ is the initial mass ratio of the binary system. $t_{\rm A}$ is time when Case A mass transfer starts, $\Delta t_{\rm f}$is the duration of the fast phase of Case A mass transfer, $\dot M_{\rm tr}^{\rm max}$ is the maximum mass transfer rate, $\Delta M_{\rm 1,f}$ and $\Delta M_{\rm 2,f}$ are mass loss of the primary and mass gain of the secondary (respectively) during fast Case A, $\Delta t_{\rm s}$ is the duration of slow Case A mass transfer, $\Delta M_{\rm 1,s}$ and $\Delta M_{\rm 2,s}$ are mass loss of the primary and mass gain of the secondary (respectively) during the slow Case A, $p_{\rm AB}$ is the orbital period at the onset of Case AB, $\Delta M_{\rm 1,AB}$ is the mass loss of the primary during Case AB (mass gain of the secondary is 1/10 of this, see Sect. 4), $M_{\rm WR,5}$ is the WR mass when the hydrogen surface abundance is $X_{\rm s}=0.05$, the WR mass at $X_{\rm s}\le 0.01$ is given in brackets, $M_{\rm O}$ is the mass of the corresponding O star, q is the mass ratio $M_{\rm WR}/M_{\rm O}$, and p is the orbital period of the WR+O system. The models are computed with a stellar wind mass loss of Hamann/6, except $^{\rm *}$ Hamann/3, $^{\rm **}$ Hamann/2.
c indicates a contact phase that occurs for low masses due to a mass ratio too far from unity, for high masses due to the secondary expansion during slow phase of Case A.
N $M_{\rm 1,in}$ $M_{\rm 2,in}$ $p_{\rm in}$ $q_{\rm in}$ $t_{\rm A}$ $\Delta t_{\rm f}$ $\dot M_{\rm tr}^{\rm max}$ $\Delta M_{\rm 1,f}$ $\Delta M_{\rm 2,f}$ $\Delta t_{\rm s}$ $\Delta M_{\rm 1,s}$ $\Delta M_{\rm 2,s}$ $p_{\rm AB}$ $\Delta M_{\rm 1,AB}$ $M_{\rm WR,5}(1)$ $M_{\rm O}$ q p
  $~{M}_{\odot}$ $~{M}_{\odot}$ $\rm d$   $10^{\rm 6}~ \rm yr$ $10^{\rm 4}~ \rm yr$ $~{M}_{\odot}/\rm yr$ $~{M}_{\odot}$ $~{M}_{\odot}$ $10^{\rm 6}~ \rm yr$ $~{M}_{\odot}$ $~{M}_{\odot}$ $\rm d$ $~{M}_{\odot}$ $~{M}_{\odot}$ $~{M}_{\odot}$   $\rm d$
N1 41 20 3 2.05 2.8 c - - - - - - - - - - - -
N2 41 20 6 2.05 3.6 3.9 5.4 18.82 1.85 0.39 0.97 0.06 5.9 7.1 11.8(11.2) 22.5 0.52 12.6
N3 41 20.5 3 2.00 2.8 2.2 18.0 21.13 2.11 - - - 2.85 8.17 7.7(7.2) 23.2 0.33 12.5
N4 41 24 3 1.71 2.8 3.1 3.6 15.18 1.51 1.51 5.13 0.20 3.87 9.05 10.1(9.3) 26.4 0.38 13.5
N5 41 24 6 1.71 3.6 4.3 3.2 17.31 1.72 0.42 1.88 0.09 8.92 7.53 12.1(11.4) 26.3 0.46 21.5
N6 41 27 3 1.52 2.75 5.8 1.9 13.82 1.37 1.51 5.86 0.17 4.38 9.59 10.3(9.8) 29.1 0.35 16.6
N7 41 30 3 1.37 2.7 6.7 1.1 12.60 1.24 1.51 6.72 0.08 5.20 9.76 10.5(10.0) 31.8 0.33 20.8
N8 45 27 3 1.67 2.5 3.6 3.3 15.41 1.53 1.57 7.48 0.25 3.88 8.81 11.5(10.7) 29.4 0.39 12.0
N9 56 33 3 1.70 1.9 5.0 4.1 17.2 1.70 1.86 15.66 0.44 4.07 7.14 13.6(12.7) 35.4 0.38 9.8
N10 56 33 6 1.70 2.8 5.8 3.1 19.35 1.9 0.60 4.77 0.02 7.77 9.18 18.6(17.5) 35.1 0.53 15.2
N11$^{\rm *}$ 56 33 6 1.70 2.8 5.8 3.1 19.35 1.9 0.46 3.63 0.06 7.91 7.15 18.6(17.2) 34.9 0.53 13.8
N12$^{\rm **}$ 56 33 6 1.70 2.8 5.8 3.1 19.35 1.9 0.43 3.43 0.07 8.89 3.5 18.3(16.4) 34.5 0.53 12.1
N13 65 37 3 1.76 1.6 3.2 4.7 18.81 1.87 c - - - - 16.2(14.8) - - -
N14 75 45 3 1.67 1.3 4.2 3.1 18.57 1.79 c - - - - 18.5(16.9) - - -


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