Rapid Growth of Intermediate-Mass Black Holes through Disk-induced Stellar Disruptions
astro-ph.GA, astro-ph.HE
Submitted: 2026-09-03
Updated: 2026-09-06
Terminology
Sources
- Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots
- Overmassive black holes and little red dots naturally form in simulations
- Pebbles to Gems: Intermediate-mass black holes in the first star clusters
- Stellar mergers and chemical element mixing: implications for the metamorphic stellar evolution in AGN disks
- Rapid formation of a very massive star >50000 $M_\odot$ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
- Conditions for Changing-Look AGNs from Accretion Disk-Induced Tidal Disruption Events
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