Supermassive Black Holes Active Galactic Nuclei Neutron Stars Accretion Disks Formation Theories Formation of Black Holes Intermediate-Mass Black Holes Primordial Black Holes Formation Hawking Radiation Intermediate Mass Black Holes Tidal Disruption Events Accretion Processes Stellar Interactions Formation and Behavior Binary Systems Mergers Feedback Mechanisms Galaxy Dynamics Supernovae Galaxy Formation Effects on Galaxies Natal Kicks Big Bang Theory Stellar-mass Black Holes Simulation Techniques Self-Gravitating Systems Massive Black Holes Black Hole Remnants Formation of Galaxies Direct Collapse Black Holes Matter Interaction Cluster Dynamics Massive Objects Gas Dynamics Interactions with Stars Mass Functions Black Hole Mergers Positron Jets Mass Distribution Compact Objects Star Formation Thermodynamics Stellar Collapse Research Challenges Cosmic Phenomena Micro-Quasars Binary Star Systems Particle Jets Sagittarius A* Black Hole Jets Galaxy Mergers Overmassive Black Holes Observational Techniques Energy Sources Binary Black Hole Mergers Exoplanets Black Hole Formation Formation and Decay Eddington Limit Gravitation Black Hole Behavior Active Galaxies Galactic Nuclei Gamma Rays Galaxy Centers Gravitational Waves Galaxy Characteristics Mass Accumulation Stellar Evolution Mass Gap Galaxy Interaction Black Hole Feedback Star Destruction Binary Black Holes Accretion Discs Energy Production Stellar-Mass Black Holes Cosmic Winds Supermassive Stars Galactic Mergers Quasars Formation Mechanisms Information Paradox Types of Black Holes Spin Dynamics Mass Ratios
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A Nature Astronomy analysis using stacked JWST COSMOS‑Web images finds faint, compact stellar hosts that point to rapid black‑hole growth in the first billion years of the universe.
