No Evidence for a Significant Evolution of M•–M. Relation in Massive Galaxies up to z ∼ 4

No Evidence for a Significant Evolution of M•–M. Relation in Massive Galaxies up to z ∼ 4

Over the past two decades, tight correlations between black hole masses ( M _• ) and their host galaxy properties have been firmly established for massive galaxies (with stellar mass $\mathrm{log}({M}_{* }/{M}_{\odot })\gtrsim 10$ ) at low- z ( z < 1), indicating coevolution of supermassive black...

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Bibliographic Details
Main Authors: Yang Sun, Jianwei Lyu, George H. Rieke, Zhiyuan Ji, Fengwu Sun, Yongda Zhu, Andrew J. Bunker, Phillip A. Cargile, Chiara Circosta, Francesco D’Eugenio, Eiichi Egami, Kevin Hainline, Jakob M. Helton, Pierluigi Rinaldi, Brant E. Robertson, Jan Scholtz, Irene Shivaei, Meredith A. Stone, Sandro Tacchella, Christina C. Williams, Christopher N. A. Willmer, Chris Willott
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Active galactic nuclei
Supermassive black holes
Active galaxies
Galaxy evolution
Online Access:https://doi.org/10.3847/1538-4357/ad973b

Internet

https://doi.org/10.3847/1538-4357/ad973b

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