A high fraction of close massive binary stars at low metallicity
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, which heavily impact the characteristics of their life-ending supernova and compact remnants. For the low-metallicity environments of high-redshift galaxies, constraints on the
Sana, H. et al.
Fecha de publicación:
9
2025