From Dense Gas Clouds to Supermassive Black Hole Seeds: Hybrid Hydro/Direct N-body Simulations of Runaway Collision-driven Intermediate-mass Black Hole Formation

A population of dense stellar systems at high redshift has recently been uncovered by JWST. To investigate the formation of supermassive black hole (SMBH) seeds in these dense environments without invoking any ad hoc seeding mechanisms, we present star cluster-scale simulations performed with an upd...

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Váldodahkkit:	Eunwoo Chung, Yongseok Jo, Ji-hoon Kim, Minyong Jung, Oh-kyoung Kwon
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2026-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Black hole physics Gravitation Hydrodynamics Star clusters Intermediate-mass black holes
Liŋkkat:	https://doi.org/10.3847/1538-4357/ae742e
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