Young Stars Massive Stars Gas Dynamics Stellar Evolution Supernovae Interstellar Medium Galaxy Evolution Molecular Clouds Nebulae Star-Forming Regions Early Universe Star Clusters Galaxy Formation Binary Stars Starburst Galaxies Companion Stars Stellar Mass Protostars Starbursts Planetary Systems Population III Stars Massive Star-Forming Regions Cold Gas Brown Dwarfs Galactic Dynamics Stellar Clusters Cosmic Evolution Mass Distribution Reionization Organic Molecules Open Clusters Tidal Dwarf Galaxies Planetary Formation Ultraviolet Radiation Neutral Hydrogen Black Hole Formation Proto-stars Gas and Dust Clouds Red Dwarf Stars Nebulas Cosmic Dust Galactic Structure Gas Clouds Gas Stripping Galaxies Primordial Chemistry Chemical Reactions Active Galactic Nuclei Clumps Compact Galaxies Rapid Star Formation Chemical Conditions Star Production Rates Stellar Dynamics Cosmic Noon Intracluster Medium Active Galaxies Stellar Movement Chamaeleon Star-Forming Complex Star Formation Histories Galaxy Assembly Star Formation Rates White Dwarfs Cosmic Processes Feedback Mechanisms Cluster Dynamics Dust Formation Molecular Cloud Formation Protoplanetary Disks Stellar Feedback Gas and Dust Interactions First Stars Gravitational Instabilities Cosmology Globular Clusters Interstellar Gas Variable Stars Galactic Evolution Quenched Galaxies Galaxy Mergers Binary Star Systems Hot Stars Starburst Regions Supernovas Universe Expansion Stellar Populations Stellar Nurseries Gas Accumulation Black Holes Molecular Hydrogen Dust Distribution Stellar Systems Orbital Mechanics Binary Systems Gravitational Forces
Multiwavelength data alongside a 3D model point to a low-power radio jet limiting star-forming gas.