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Table 1.

Properties of selected models which are highlighted in Fig. 1.

Pi qi RLOF L Teff R ℒ Ys MHe − core Menv MH ΔMRLOF, C M ˙ RLOF , C M ˙ wind CC $ \left.\frac{\dot{M}_{\mathrm{RLOF,C}}}{\dot{M}_{\mathrm{wind}}}\right|_{\mathrm{CC}} $ M ˙ RLOF , C max $ \dot{M}_{\mathrm{RLOF,C}}^{\mathrm{max}} $ Δ t RLOF , C max $ \Delta t_{\mathrm{RLOF,C}}^{\mathrm{max}} $ τCE SN Einteract/ELC
(d) (k L⊙) (kK) (R⊙) (k ℒ⊙) (M⊙) (M⊙) (M⊙) (M⊙) (M⊙ yr−1) (kyr) (kyr) Type
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17) (18)
562 ( * ) 0.95 B 49.2 24.7 12.1 14.4 0.98 3.42 0.00 0.00 0.00 n.a. n.a. n.a. n.a. Ib n.a.
631 0.95 B 60.5 4.45 415 15.9 0.71 3.67 0.12 0.02 0.00 n.a. n.a. n.a. n.a. IIb n.a.
708 0.95 B 64.0 3.69 620 16.3 0.48 3.73 0.19 0.06 0.00 n.a. n.a. n.a. n.a. IIb n.a.
794 0.95 BC 65.1 3.46 710 16.0 0.44 3.78 0.28 0.12 0.01 0.44 2.1 × 10−6 2.73 n.a. IIb 0.02
891 ( * ) 0.95 BC 65.1 3.39 741 15.7 0.41 3.82 0.31 0.15 0.06 1.03 8.1 × 10−6 4.31 n.a. IIL 0.46
1000 0.95 BC 62.1 3.30 763 14.6 0.39 3.86 0.39 0.20 0.17 1.70 1.2 × 10−5 3.25 n.a. IIL 1.7
1122 0.95 BC 67.0 3.27 806 15.4 0.37 3.88 0.46 0.25 0.26 2.45 1.5 × 10−5 15.2 n.a. IIL 2.5
1259 0.95 BC 67.8 3.22 839 15.1 0.36 3.88 0.60 0.34 0.39 2.77 2.1 × 10−5 18.4 n.a. IIL 3.4
1413 0.95 BC 68.2 3.15 878 14.4 0.34 3.90 0.84 0.50 0.66 3.58 3.5 × 10−5 21.8 n.a. IIL 5.2
1585 0.95 BC 69.2 3.09 917 13.5 0.32 3.92 1.18 0.73 1.06 5.18 5.9 × 10−5 23.7 n.a. IIP 7.1
1778 0.95 BC 70.0 3.05 950 12.3 0.31 3.95 1.73 1.11 1.90 6.83 1.2 × 10−4 25.8 n.a. IIP 9.9
1995 0.95 C 71.5 3.03 970 10.5 0.30 3.98 2.80 1.85 4.06 13.0 5.9 × 10−4 21.2 n.a. IIP 14
2239 0.95 C 71.1 3.05 958 9.18 0.30 3.98 3.74 2.50 3.11 20.1 4.2 × 10−4 11.5 n.a. IIP 10
2512 ( * ) 0.95 C 71.1 3.12 916 7.12 0.30 3.98 5.97 4.03 0.88 80.4 5.5 × 10−4 1.12 n.a. IIP 2.6
2818 0.95 No 71.1 3.15 898 6.54 0.30 3.98 6.86 4.64 0.00 n.a. n.a. n.a. n.a. IIP n.a.
2512 0.90 C 70.9 3.11 919 7.30 0.30 3.98 5.70 3.84 1.16 106 8.1 × 10−4 1.16 n.a. IIP 0.003
2512 0.85 C 71.2 3.10 928 7.57 0.30 3.98 5.40 3.64 1.45 152 1.3 × 10−3 1.12 n.a. IIP 0.004
2512 0.80 C 71.3 3.09 935 7.86 0.30 3.98 5.06 3.40 1.79 263 1.6 × 10−3 1.06 n.a. IIP 0.005
2512 0.75 C 71.7 3.10 929 7.55 0.30 3.98 5.48 3.70 1.37 1106 4.4 × 10−3 0.00 n.a. IIP 0.006
2512 0.70 C 71.2 3.14 902 6.64 0.30 3.98 6.71 4.54 0.14 51.9 1.9 × 10−4 0.00 n.a. IIP 0.004
2512 0.65 C 71.2 3.15 900 6.57 0.30 3.98 6.82 4.62 0.03 5.54 2.1 × 10−5 0.08 n.a. IIP 0.00
2512 0.60 No 71.1 3.15 898 6.54 0.30 3.98 6.84 4.63 0.009 n.a. n.a. n.a. n.a. IIP n.a.
2512 0.55 No 70.9 3.15 897 6.52 0.30 3.98 6.85 4.64 0.00 n.a. n.a. n.a. n.a. IIP n.a.
2512 0.50 No 71.1 3.15 898 6.54 0.30 3.98 6.86 4.64 0.00 n.a. n.a. n.a. n.a. IIP n.a.
1995 0.90 C 70.9 3.03 968 10.8 0.30 3.98 2.56 1.68 4.30 12.8 9.1 × 10−4 21.3 n.a. IIP 14
1995 0.85 C 71.1 3.03 968 11.2 0.31 3.98 2.33 1.52 4.53 11.6 1.5 × 10−3 21.3 n.a. IIP 15
1995 0.80 C 70.7 3.04 963 11.7 0.31 3.98 2.06 1.34 4.81 10.4 4.0 × 10−3 21.2 n.a. IIP 16
1995 0.75 C 71.0 3.05 957 12.3 0.31 3.98 1.76 1.13 5.10 9.38 1.3 × 10−2 21.0 n.a. IIP 17
1995 0.70 C 71.2 3.07 944 13.1 0.32 3.98 1.42 0.90 5.43 8.54 3.3 × 10−2 20.3 n.a. IIP 18
1995 0.65 C 70.9 3.11 918 14.0 0.33 3.98 1.08 0.67 5.78 6.60 7.9 × 10−2 19.8 n.a. IIP 19
1995 0.60 C 70.7 3.18 879 14.9 0.34 3.98 0.74 0.44 6.12 5.12 0.14 18.7 n.a. IIL 21
1995 0.55 C 71.1 3.29 821 16.0 0.38 3.98 0.45 0.25 6.40 3.40 0.20 17.7 n.a. IIL 22
1995 0.50 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 4.1 2.72 ? 0.25 16.4 19.6 II ∼9 − 23
1995 0.45 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 4.5 2.33 ? 0.29 14.8 22.5 II ∼8 − 23
1995 0.40 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 4.8 2.08 ? 0.32 13.0 26.0 II ∼7 − 23
1995 0.35 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 5.0 1.87 ? 0.35 10.7 30.3 II ∼6 − 23
1995 0.30 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 5.2 1.70 ? 0.39 7.58 36.3 II ∼6 − 23
1995 0.25 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 5.3 1.54 ? 0.43 3.50 42.9 II ∼5 − 23
1995 0.20 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 5.4 1.42 ? 0.48 0.74 52.7 II ∼5 − 23
1995 0.15 No 71.1 3.15 899 6.54 0.30 3.98 6.85 4.63 0.00 n.a. n.a. n.a. n.a. IIP n.a.
1995 0.10 No 71.0 3.15 898 6.53 0.30 3.98 6.86 4.64 0.00 n.a. n.a. n.a. n.a. IIP n.a.
1413 0.90 BC 66.7 3.18 854 14.4 0.35 3.89 0.71 0.42 0.54 3.19 2.9 × 10−5 20.6 n.a. IIL 4.4
1413 0.85 BC 67.4 3.22 835 15.1 0.36 3.88 0.59 0.33 0.39 2.68 2.1 × 10−5 18.5 n.a. IIL 3.5
1413 0.80 BC 66.8 3.27 808 15.3 0.37 3.87 0.48 0.26 0.26 2.06 1.4 × 10−5 15.3 n.a. IIL 2.5
1413 0.75 BC 66.7 3.30 790 15.6 0.38 3.86 0.42 0.22 0.21 1.93 1.3 × 10−5 3.25 n.a. IIL 2.1
1413 0.70 BC 65.2 3.40 737 15.8 0.40 3.81 0.31 0.15 0.03 0.86 5.0 × 10−6 3.44 n.a. IIL 0.33
1413 0.65 B 63.8 3.51 685 15.9 0.43 3.76 0.25 0.10 0.00 n.a. n.a. n.a. n.a. IIb n.a.
1413 0.60 B Common envelope evolution ≳0.30 ∼4 ∼11 0.00 n.a. n.a. n.a. 4.58 II n.a.
⋮
1413 0.15 B Common envelope evolution ≳0.30 ∼4 ∼7 0.00 n.a. n.a. n.a. 20.0 II n.a.
1413 0.10 C Common envelope evolution ≳0.30 3.98 ∼0.2 − 5.7 1.17 ? 0.91 20.2 31.6 II ∼4 − 23

Notes. The models are identified by their initial orbital period (Col. 1), initial mass ratio (2), and mass transfer case (3). Further, we give the properties of the primary stars at core collapse, namely luminosity (4), effective temperature (5), radius (6), spectroscopic luminosity (7), surface helium mass fraction (8), helium core mass (9), envelope mass (10) and the mass of hydrogen in the envelope (11). Column 12 shows the amount of mass lost via RLOF during stable Case C mass transfer. Column 13 shows the ratio between the Case C mass transfer rate and wind mass-loss rate at the time of collapse, averaged over the last 100 years. Columns 14 and 15 give the maximum mass transfer rate occurring during Case C RLOF alongside the time before collapse at which it is found. Column 16 shows the estimated timescale for common-envelope evolution (see Eq. (4)) when applicable. Column 17 displays the expected SN type if no CSM interaction would occur, and Col. 18 estimates the energy expected to be thermalized by the CSM interaction (Einteract, see Eq. (5)), divided by the radiated energy of the SN when the interaction is neglected (ELC ∼ 3 × 1049 erg; Dessart et al. 2024). ( * )Model did not reach core collapse but terminated after core silicon exhaustion.

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