Feedback from Pop III.1 stars creates HII regions of radius 1.3 cMpc, regulating their isolation and producing an SMBH density of 0.2 cMpc^{-3} with most forming at z~20.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback
Feedback from Pop III.1 stars creates HII regions of radius 1.3 cMpc, regulating their isolation and producing an SMBH density of 0.2 cMpc^{-3} with most forming at z~20.