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Table 1

Properties of our set of progenitor models.

Model Mi Mf MFe,c MCO,c log L R M(He) M(C) M(N) M(O) Xs(He) Xs(C) Xs(N) Xs(O)
[M] [M] [M] [M] [L] [R] [M] [M] [M] [M]
he4 4.0 2.98 1.46 1.82 4.57 7.97 1.133 0.056 0.009 0.150 0.980 0.000 0.013 0.000
he5 5.0 3.56 1.47 2.29 4.79 3.60 1.195 0.110 0.008 0.423 0.980 0.000 0.013 0.000
he6 6.0 4.07 1.80 2.71 4.92 2.46 1.160 0.227 0.006 0.571 0.980 0.000 0.013 0.000
he7 7.0 4.55 1.63 3.13 5.01 1.51 1.075 0.352 0.005 0.838 0.980 0.000 0.013 0.000
he8 8.0 5.00 1.64 3.55 5.09 1.23 0.935 0.503 0.003 1.214 0.980 0.000 0.013 0.000

he9 9.0 5.29 1.57 3.93 5.12 0.87 0.628 0.659 0.000 1.487 0.822 0.148 0.000 0.005

he10 10.0 5.20 1.67 4.06 5.16 0.46 0.327 0.678 0.000 1.580 0.452 0.452 0.000 0.071
he11 11.0 5.25 1.55 4.01 5.12 0.59 0.220 0.674 0.000 1.659 0.295 0.525 0.000 0.155
he12 12.0 5.43 1.67 4.11 5.20 0.49 0.236 0.763 0.000 1.831 0.195 0.530 0.000 0.251

Notes. Models he4-he8 (he10-he12) correspond to SNe Ib (Ic) progenitors. Model he9 is an intermediate case. For each progenitor model, the table gives the initial mass Mi, the final mass Mf, the Fe-core mass (where the electron fraction first rises to 0.499 from the center), the CO-core mass (outermost location where the He mass fraction is lower than 0.01), the final surface luminosity log L, the final surface radius R, followed by the total mass of He, C, N, O, as well as the surface mass fraction of He, C, N, and O.

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