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Table 1

Properties of the models evolved with mesa, some corresponding to the initial conditions on the ZAMS and others to the onset of core collapse.

Model Zinit Ω/Ωcrit Age Teff L R Mfinal MSi,c MFe,c XHe,s XC,s XN,s XO,s XSi,s
[Myr] [kK] [L] [R] [M] [M] [M]

r0 0.0162 0 5.06 166 3.39(5) 0.70 11.4 1.59 1.57 1.88(–1) 5.14(–1) 0.0 2.79(–1) 5.03(–4)
r4 0.0162 0.4 5.44 200 3.28(5) 0.48 10.0 2.01 1.82 1.75(–1) 5.20(–1) 0.0 2.86(–1) 5.03(–4)
r6 0.0162 0.6 6.25 146 1.79(5) 0.67 6.6 1.67 1.55 2.91(–1) 5.38(–1) 0.0 1.52(–1) 5.02(–4)
r6z 0.002 0.6 7.37 145 2.88(5) 0.86 9.7 2.15 1.87 9.98(–1) 8.57(–5) 1.55(–3) 2.41(–5) 3.76(–5)

Notes. All models start from a 40 M star on the ZAMS, but with different initial rotation rates and metallicities.

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