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...
Main Authors: | , , , , , , , , |
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Format: | Article |
Language: | English |
Published: |
Oxford University Press (OUP),
2022-05-06T16:13:49Z.
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Subjects: | |
Online Access: | Get fulltext |