Science ❯ Astronomy ❯ Astrophysics
Protostars Protoplanetary Disks Young Stars Massive Stars Brown Dwarfs Supernovae Molecular Clouds James Webb Space Telescope Nebulae Supermassive Black Holes Planetary Formation Giant Stars Herbig-Haro Objects Starburst Galaxies Proto-stars CO-dark Molecular Gas Star Clusters Life in the Universe Shock Waves Dust in Galaxies Gas Dynamics Planet Formation Black Hole Activity Dust Production Planetary Nebulae Magnetic Fields 30 Doradus Cosmic Dust Dwarf Galaxies Galaxy Morphology Computational Simulations Celestial Objects Interstellar Gas NGC 346 Molecular Hydrogen Cooling Metal-Rich Stars Baby Stars Research Methodology Planetary System Formation Stellar Families Giant Molecular Clouds Infant Stars Atomic Hydrogen Gas Proto Stars Ionized Hydrogen Regions Hubble Space Telescope Protoplanetary Discs Planetary Systems Early Stars Sagittarius B2 Star Formation Rates Red Dwarfs Cosmic Noon Low Surface Brightness Galaxies Pismis 24 High-Mass Stars Protoplanets Star Spots Stellar Evolution Embedded Sources Protostellar Jets Stellar Nurseries Star-Formation Histories 3D Mapping Gas and Dust Clouds Neutral Hydrogen Supernova Mechanisms Radio Astronomy Galactic Starbursts Supernova Enrichment Polycyclic Aromatic Hydrocarbons HII Regions Galactic Feedback Planetary Evolution Extragalactic Studies Circumstellar Disks Organic Molecules HOPS-315 Gravitational Interaction Thermonuclear Reactions Galactic Structures Supernova Frequency Galactic Evolution Rogue Worlds Gas Clouds Galaxy Evolution Solar Systems Companion Stars Orbital Dynamics Chemical Enrichment Milky Way
Multiwavelength data alongside a 3D model point to a low-power radio jet limiting star-forming gas.