The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction

@article{Zapartas2019TheDL,
title={The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction},
author={Emmanouil Zapartas and Selma E. de Mink and Stephen Justham and Nathan Smith and Alexander de Koter and Mathieu Renzo and Iair Arcavi and Robert Farmer and Ylva G{\"o}tberg and Silvia Toonen},
journal={Astronomy \& Astrophysics},
year={2019}
}
Hydrogen-rich supernovae, known as Type II (SNe II), are the most common class of explosions observed following the collapse of the core of massive stars. We used analytical estimates and population synthesis simulations to assess the fraction of SNe II progenitors that are expected to have exchanged mass with a companion prior to explosion. We estimate that 1/3 to 1/2 of SN II progenitors have a history of mass exchange with a binary companion before exploding. The dominant binary channels…
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