Overmassive black holes and little red dots naturally form in simulations
astro-ph.GA, astro-ph.CO, astro-ph.SR
Submitted: 2026-01-08
Updated: 2026-09-18
Comments: Published in Nature 657, 621--625 (2026); 14 figures
Journal ref: Nature 657, 621--625 (2026)
DOI: 10.1038/s41586-026-10985-8
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties
- GA-NIFS: A massive black hole in a low-metallicity AGN at $z\sim5.55$ revealed by JWST/NIRSpec IFS
- JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty
- A small and vigorous black hole in the early Universe
- Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots
- Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys
- RUBIES: A Spectroscopic Census of Little Red Dots; All V-Shaped Point Sources Have Broad Lines
- Little red dots as young supermassive black holes in dense ionized cocoons
- A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots
- RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec
- Sustained super-Eddington accretion in high-redshift quasars
- Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe
- Little Red Dots and their Progenitors from Direct Collapse Black Holes
- Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$
- High-redshift AGN population in radiation-hydrodynamics simulations
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- A Semi-analytic Framework of Population III and Subsequent Galaxy Formation on Cosmological N-body Simulations
- Radiation hydrodynamics simulations of the formation of direct-collapse supermassive stellar systems
- Formation of massive black holes in rapidly growing pre-galactic gas clouds
- The Formation of Very Massive Stars in Early Galaxies and Implications for Intermediate Mass Black Holes
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