Image Details
Caption: Figure 8.
Cumulative distribution of the time between the onset of mass transfer and core collapse, ﹩\mathrm{log}({\rm{\Delta }}{t}_{\mathrm{RLOF}-\mathrm{CC}}﹩ yr −1), estimated for a 20 M ⊙ RSG progenitor evolving in a binary with a 1/10 as a massive companion, shown for different metallicities.
© 2022. The Author(s). Published by the American Astronomical Society.