Binary stars in the Milky Way nuclear stellar cluster
Context. Intermediate mass galaxies, including the Milky Way, typically host both a supermassive black hole (SMBH) and a nuclear stellar cluster (NSC). Binary systems residing in an NSC evolve dynamically via frequent close encounters with surrounding stars and secular processes related to the SMBH. Aims. Although the evolution of very soft and very hard binaries can be predicted semi-analytically
