This test case evolves a very massive helium star from the He-ZAMS up to the ocurrence of a pulsational pair-instability event (see Marchant et al. 2019).
Initialization of the model¶
The initial mass of the helium star is set in
In this case we use a \(72 M_\odot\)
Last-Updated: 2019-11-12 (mesa r12413) by Pablo Marchant