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Table 8

Properties of the subset of models run to the onset of core collapse, defined as the time when max { | v | } ≥ 103 km s-1.

Onset of core collapse: max { | v | } ≥ 103 km s-1

MZAMS [ M ] η ID M4 [ M ] μ 4 Mρ6 [ M ] MCO [ M ] MFe [ M ]

15 1.0 V-NJ 0.103 1.71 0.045 1.68 2.91 1.39
K-vL 0.132 1.78 0.051 1.79 3.07 1.50

25 0.33 V-vL 0.227 1.73 0.084 1.84 6.38 1.51
K-dJ 0.308 2.05 0.100 2.19 6.40 1.63

30 0.33 V-dJ 0.358 1.60 0.163 2.21 7.98 1.56
K-NJ 0.276 1.82 0.100 1.98 7.90 1.58

Notes. M4 and μ4 are the parameters used to predict the SN outcome of a stellar model in Ertl et al. (2016), see also text. is the mass enclosed in the location where the density drops below 106 g cm-3, MCO and MFe are the carbon-oxygen and iron core masses, respectively.

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