Chemical Abundances in High-Mass X-ray Binaries
In recent years, gravitational waves (GWs) have been detected from various sources, including black hole (BH) and neutron star (NS) mergers, posing new challenges to our understanding of massive stellar evolution. Although numerous population synthesis models have been presented to explain these events, their results depend on many parameters
Caballero-Almagro, A. et al.
Fecha de publicación:
5
2025