Impact of gas-based seeding on supermassive black hole populations at z ≥ 7

Impact of gas-based seeding on supermassive black hole populations at z ≥ 7

Deciphering the formation of supermassive black holes (SMBHs) is a key science goal for upcoming observational facilities. In many theoretical channels proposed so far, the seed formation depends crucially on local gas conditions. We systematically characterize the impact of a range of gas-based bla...

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Bibliographic Details
Main Authors: Bhowmick, Aklant K, Blecha, Laura, Torrey, Paul, Kelley, Luke Zoltan, Vogelsberger, Mark, Kosciw, Kaitlyn, Nelson, Dylan, Weinberger, Rainer, Hernquist, Lars
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: Oxford University Press (OUP) 2022
Online Access:https://hdl.handle.net/1721.1/142394

Internet

https://hdl.handle.net/1721.1/142394

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