The Redshift Evolution of the MBH–M* Scaling Relation: New Insights from Cosmological Simulations and Semianalytic Models

We study the coevolution of black holes (BHs) and their host galaxies in the A STRID and TNG300 cosmological simulations and the D ARK S AGE semianalytic model (SAM), focusing on the evolution of the BH mass–stellar mass ( M _BH – M _* ) relation. Due to differences in the adopted subgrid modeling o...

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Bibliographic Details
Main Authors: Shashank Dattathri, Priyamvada Natarajan, Antonio J. Porras-Valverde, Colin J. Burke, Nianyi Chen, Tiziana Di Matteo, Yueying Ni
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adbeef
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