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Table 4

Properties of the models at the end of their evolution.

Mini vini/vcrit MHe1 MCO Mrem (baryon./grav.) Tot. Ej. H He Prog. type SN type2 Remnant Ppuls
M M M M M M M s

120 0 (30.91) 30.13 9.13 / 4.51 21.72 0.00 0.67 WC Ib BH
0.4 (19.04) 18.46 5.69 / 3.65 13.29 0.00 0.52 WC Ic BH
85 0 (18.65) 17.98 5.54 / 3.60 13.09 0.00 0.47 WC Ic BH
0.4 (26.39) 25.72 7.88 / 4.26 18.47 0.00 0.61 WC Ib BH
60 0 (12.50) 12.23 3.91 / 2.91 8.57 0.00 0.42 WC Ic BH
0.4 (17.98) 17.52 5.40 / 3.55 12.58 0.00 0.50 WC Ic+coll.? BH
40 0 (12.82) 10.08 3.40 / 2.64 9.41 0.00 0.95 WNE Ib NS
0.4 (12.33) 12.21 3.90 / 2.90 8.42 0.00 0.41 WC Ic+coll.? BH
32 0 (10.92) 8.49 3.02 / 2.42 7.89 0.00 2.29 WNE Ib NS
0.4 (10.13) 10.01 3.38 / 2.63 6.73 0.00 0.28 WC Ic NS 1.3 × 10-4
25 0 8.12 5.95 2.41 / 2.03 5.85 0.03 2.20 WNL II-L/b NS
0.4 9.69 7.09 2.69 / 2.22 6.99 0.00 1.59 WC Ib NS 7.9 × 10-5
20 0 6.21 4.00 1.91 / 1.68 6.66 1.15 3.31 RSG II-L/b NS
0.4 7.17 4.73 2.10 / 1.82 5.06 0.02 1.61 WNL II-L/b NS 9.7 × 10-5
15 0 4.25 2.41 1.50 / 1.37 11.72 5.81 4.82 RSG II-P NS
0.4 5.11 3.19 1.71 / 1.53 9.36 3.31 3.75 RSG II-P NS 9.2 × 10-5
12 0 2.99 1.75 1.33 / 1.23 9.97 5.64 3.75 RSG II-P NS
0.4 3.90 2.34 1.48 / 1.35 8.73 4.02 3.31 RSG II-P NS 9.5 × 10-5
9 0 1.21 1.20 1.12 / 1.05 7.64 4.58 2.87 RSG II-P NS
0.4 3.08 1.64 1.30 / 1.20 7.22 3.53 3.03 RSG II-P NS 1.2 × 10-4

Notes. The columns are: the initial mass (Col. 1), the initial velocity (Col. 2), the final masses of the He (Col. 3) and CO (Col. 4) cores, the baryonic and gravitational mass of the remnant (Col. 5), the total mass of the ejecta (Col. 6), the ejected mass of H (Col. 7) and He (Col. 8), the progenitor type (Col. 9), the SN type (Col. 10), the remnant type (Col. 11) and the pulsation period of the NS (Col. 12).

(1)

The parenthesis indicates that the value corresponds to the whole stellar mass.

(2)

The SN types given here are determined using the “medium SN Ic” criterion . The models that might lead to a LGRB through a collapsar event are indicated by the label “coll.?” (see text).

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