Stronger stellar feedback lowers central stellar densities in low-mass merger remnants and systematically lengthens SMBH merger delays, yielding a 30–500 Myr spread in post-hardening coalescence times.
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RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime
Stronger stellar feedback lowers central stellar densities in low-mass merger remnants and systematically lengthens SMBH merger delays, yielding a 30–500 Myr spread in post-hardening coalescence times.