Formation of Heavy Seed Black Holes and Little Red Dots-like Compact Clusters in Metal-enriched Star-forming Regions
astro-ph.GA, astro-ph.CO
Submitted: 2026-08-31
Updated: 2026-08-31
Comments: 19 pages, 13 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Double Dots: Compact Pairs Mark Little Red Dots and High-Redshift Broad-line AGNs
- Overmassive black holes and little red dots naturally form in simulations
- SAPPHIRES: Extremely Metal-Poor Galaxy Candidates with $12+{\rm log(O/H)}<7.0$ at $z\sim5-7$ from Deep JWST/NIRCam Grism Observations
- Pristine Massive Star Formation Caught at the Break of Cosmic Dawn
- DREAMS.II. Galaxy Demographics from Direct Te-Based Metallicities at z~2-10: Tracing the Evolution of the Mass-Metallicity and Fundamental Relations
- SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds
- Hidden in Pixels. I. Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales
- VENUS: Two Faint Little Red Dots Separated by $\sim70\,\mathrm{pc}$ Hidden in a Single Lensed Galaxy at $z\sim7$
- Little red dot variability over a century reveals black hole envelope via a giant Einstein cross
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