Active Galactic Nuclei Galactic Dynamics Star Formation Sagittarius A* Orbital Dynamics Galaxy Evolution Cosmic Horseshoe Infinity Galaxy Galactic Mergers Observational Astronomy Gas Outflows Galaxy Mergers Growth of Black Holes Behavior of Supermassive Black Holes Black Hole Awakening Black Hole Behavior Feeding Processes Galactic Evolution Little Red Dots Porphyrion Matter Accretion Formation Theories Event Horizon Accretion Disks Active Supermassive Black Holes GN-z11 Black Hole Seeds Accretion Processes Mapping Messier 83 Sombrero Galaxy Black Hole Gravitational Effects Radiation Effects Dark Matter Radio Astronomy CAPERS-LRD-z9 Galaxy Clusters Galactic Collisions Galaxy Collisions Thermal Characteristics Observational Studies Black Hole Feeding Early Universe Galaxy Formation Milky Way Cosmic Winds Orphan Black Holes Galactic Phenomena Ultramassive Galaxies Growth Mechanisms
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A new three-dimensional diagnostic applied to VLT/MUSE and Chandra data shows shocks from jet–ISM or wind–ISM interactions are widespread and may help shape circumnuclear star formation.
