Compact object mergers: Observations of supermassive binary black holes and stellar tidal disruption events
S. Komossa, J.A. Zensus

TL;DR
This paper reviews the current observational status of supermassive black hole binaries, their role in galaxy evolution, and stellar tidal disruption events, highlighting their importance for understanding gravitational waves and black hole growth.
Contribution
It provides a comprehensive overview of observational evidence and implications of SMBH pairs, binaries, and TDEs, emphasizing their significance in astrophysics and gravitational wave research.
Findings
Identification of SMBH pairs and binaries informs galaxy merger processes.
Stellar TDEs are luminous transients useful for astrophysical studies.
Future surveys will detect thousands of TDEs, expanding their scientific utility.
Abstract
The capture and disruption of stars by supermassive black holes (SMBHs), and the formation and coalescence of binaries, are inevitable consequences of the presence of SMBHs at the cores of galaxies. Pairs of active galactic nuclei (AGN) and binary SMBHs are important stages in the evolution of galaxy mergers, and an intense search for these systems is currently ongoing. In the early and advanced stages of galaxy merging, observations of the triggering of accretion onto one or both BHs inform us about feedback processes and BH growth. Identification of the compact binary SMBHs at parsec and sub-parsec scales provides us with important constraints on the interaction processes that govern the shrinkage of the binary beyond the "final parsec". Coalescing binary SMBHs are among the most powerful sources of gravitational waves (GWs) in the universe. Stellar tidal disruption events (TDEs)…
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