Pre-SN progenitor properties for our model set. MH,e refers to the H-rich envelope in the type II SN models.
|Type II SN progenitors|
Notes. The He, CO, and Si core masses correspond to Lagrangian masses. (a) The type II SN model m12 has a total mass greater than the initial mass by 0.4 M⊙ because of the adopted H-rich envelope mass. Its core properties are, however, compatible with the results from our MESA grid. Such a model couldarise from a merger (Menon & Heger 2017).
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