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This document discusses the delay time distribution (DTD) of tidal disruption flares, which can help distinguish between proposed mechanisms for the overrepresentation of tidal disruption events (TDEs) in post-starburst galaxies. It finds that supermassive black hole binaries are an unlikely explanation, as they predict an unrealistic mass distribution and require extensive fine-tuning to match observations. Steep central stellar density profiles created during a starburst can reasonably match the observed
- Author
- Luciano Del Valle
- Language
- EN