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 (Author), Blecha, Laura (Author), Torrey, Paul (Author), Kelley, Luke Zoltan (Author), Vogelsberger, Mark (Author), Kosciw, Kaitlyn (Author), Nelson, Dylan (Author), Weinberger, Rainer (Author), Hernquist, Lars (Author)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2022-05-06T16:13:49Z.
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