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Table 1

Properties of single stellar models for different initial masses Mi.

Mi Mf MH Teff SN type
(M) (M) (M) (103 K)

32 13.94 1.014 5.56 3.6 IIL
32.5 12.89 0.505 5.57 3.8 IIb
33 11.81 0.080 5.58 4.3 Ib

Notes. The final mass Mf and the amount of hydrogen in the envelope MH are given at the time of explosion, together with the luminosity log(L/L) and effective temperature Teff at the onset of central carbon burning.

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