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Table A.1.

Pre-SN and SN explosion properties of the presented stellar models.

Mini Case facc tcc Mcc MCO sc SN Mrm Mej MH, env Fall- log Lcc log Teff, cc Rcc δtLBV Eexpl MNi vkick
(M) (Myr) (M) (M) (NAkB) Type (M) (M) (M) back? (log L) (log K) (R) (104 yr) (1051 erg) (M) (km s−1)
11.0 Single 22.4 10.0 2.0 0.78 II 1.30 8.6 6.8 0 4.76 3.52 718 0.0 0.45 0.02 216
11.0 Case A-e 0.10 21.6 11.0 2.1 0.81 II 1.33 9.6 7.6 0 4.80 3.52 757 0.0 0.98 0.04 507
11.0 Case A-e 0.25 21.6 12.0 2.8 0.86 II 1.42 10.4 7.9 0 4.95 3.52 912 0.0 0.96 0.05 479
11.0 Case A-e 0.50 21.5 13.0 3.9 0.90 II 1.45 11.3 7.3 0 5.12 3.53 1059 0.0 0.70 0.05 343
11.0 Case A-e 0.75 21.0 13.3 5.3 0.91 II 1.46 11.6 6.2 0 5.28 3.57 1076 0.0 2.18 0.14 1426
11.0 Case A-e 1.00 20.6 13.1 6.6 1.14 BH 13.1 0.0 4.6 0 5.40 3.61 1013 0.0 0.00 0.00 0
11.0 Case A-e 1.50 20.1 14.1 9.3 0.95 II 1.59 12.3 2.6 0 5.62 3.73 758 1.4 1.07 0.13 631
11.0 Case A-e 2.00 19.6 16.0 12.4 1.05 II 1.73 14.0 1.2 0 5.76 4.12 148 48.7 1.72 0.17 993

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Notes. The provided data are the initial mass, Mini, the model case (single or accretor including an indication of the evolutionary stage at accretion), the fraction, facc, of accreted mass in units of Mini, the lifetime, tcc, until core collapse, the final stellar mass, Mcc, the CO core mass, MCO, at core collapse, the central entropy, sc, at core collapse, the SN type, the gravitational compact-object remnant mass, Mrm, the SN ejecta mass, Mej, the mass of the hydrogen-rich envelope, MH, env, of the SN progenitor, a flag indicating the likely occurrence of SN fallback, the luminosity, log Lcc, effective temperature, Teff, cc, and radius, R*, at core collapse, the time, δtLBV, spent in the LBV-region of the HR diagram, the SN explosion energy, Eexpl, the ejected nickel mass, MNi, and the SN kick velocity, vkick, of a formed NS. The full table is available in electronic form at the CDS and via Zenodo at https://doi.org/10.5281/zenodo.15791044.

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