A population synthesis with detailed binary grids shows stripped-envelope supernovae mostly come from primary stars stripped by stable mass transfer, with a flat total rate across metallicity but strong subtype variation.
@doi [ ] 10.3847/1538-4357/ad284e, https://ui.adsabs.harvard.edu/abs/2024ApJ...964...56D 964
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The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity
A population synthesis with detailed binary grids shows stripped-envelope supernovae mostly come from primary stars stripped by stable mass transfer, with a flat total rate across metallicity but strong subtype variation.