Kavli Affiliate: J. S. Villasenor| First 5 Authors: H. Sana, H. Sana, , , | Summary:At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, heavily impacting the characteristics of their life-ending supernova and compact remnants. For the low-metallicity […]
Continue.. A high fraction of close massive binary stars at low metallicity