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Table 3

Surface chemical composition and comparison of spectral types of core-collapse SN progenitor with previous studies.

Mini Xsurf Ysurf Csurf Nsurf Osurf Previous Sp. Typea New Sp. Type SN typea
(M) (mass) (mass) (mass) (mass) (mass) (Chem. Abund.)

non-rotating models
9 0.68 0.31 1.6 × 10-3 3.0 × 10-3 4.4 × 10-3 RSG K − M  I IIP
12 0.68 0.31 1.3 × 10-3 2.5 × 10-3 4.8 × 10-3 RSG K − M  I IIP
15 0.65 0.34 1.1 × 10-3 3.2 × 10-3 4.4 × 10-3 RSG K − M  I IIP
20 0.48 0.51 8.4 × 10-5 6.9 × 10-3 1.6 × 10-3 RSG K − M  I IIL/b
23 0.31 0.67 6.4 × 10-5 8.1 × 10-3 1.5 × 10-4 RSG K − M  I IIL/b
25 0.16 0.83 6.8 × 10-5 8.2 × 10-3 1.1 × 10-4 WNL WN11h/LBV IIL/b
32 0.00 0.99 1.4 × 10-4 8.1 × 10-3 1.0 × 10-4 WNE WN 7–8o Ib
40 0.00 0.99 9.5 × 10-5 8.2 × 10-3 9.2 × 10-5 WNE WN 7–8o Ib
50 0.00 0.19 0.46 1.5 × 10-5 0.33 WC WO 1–3 Ib
60 0.00 0.27 0.51 0.00 0.20 WC WO 1–3 Ic
85 0.00 0.25 0.49 0.00 0.25 WC WO 1–3 Ic
120 0.00 0.24 0.46 0.00 0.29 WC WO 1–3 Ib

rotating models, initial υrot/υcrit = 0.4
9 0.64 0.35 6.2 × 10-4 3.8 × 10-3 4.4 × 10-3 RSG K − M  I IIP
12 0.64 0.35 6.2 × 10-4 3.9 × 10-3 4.2 × 10-3 RSG K − M  I IIP
15 0.56 0.43 4.9 × 10-4 4.7 × 10-3 3.5 × 10-3 RSG K − M  I IIP
16.5 0.55 0.44 4.8 × 10-4 4.8 × 10-3 3.4 × 10-3 RSG K − M  I IIP
18 0.38 0.61 4.9 × 10-5 7.0 × 10-3 1.4 × 10-3 RSG G1Ia+ IIL/b
20 0.24 0.75 6.2 × 10-5 7.8 × 10-3 4.9 × 10-4 WNL LBV IIL/b
25 0.03 0.93 1.6 × 10-4 1.6 × 10-3 6.5 × 10-4 WNL LBV Ib
28 0.00 0.97 9.3 × 10-3 1.0 × 10-2 1.2 × 10-3 WNL WN 10–11 Ib
32 0.00 0.28 0.47 2.2 × 10-3 0.23 WC WO 1 Ic
40 0.00 0.28 0.50 4.0 × 10-5 0.20 WC WO 1-2 Ic
60 0.00 0.28 0.49 0.00 0.21 WC WO 1-3 Ic
85 0.00 0.26 0.47 0.00 0.25 WC WO 1-3 Ib
120 0.00 0.26 0.49 0.00 0.23 WC WO 1 Ic

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