Nebulae Young Stars Protostars Stellar Evolution Star-Forming Regions Star Clusters Massive Stars Stellar Nurseries Protoplanetary Disks Magnetic Fields Molecular Clouds Supernovae Protostellar Outflows New Star Formation Gas Clouds Gas Dynamics New Stars Starburst Galaxies Cosmic Dust Early Universe Nebulas Star-Forming Region Starburst Active Star Formation Super Star Clusters Orion Nebula Bipolar Jets Tarantula Nebula Planet Formation Low-Mass Stars Interstellar Medium Galactic Characteristics Companion Stars Cosmic Time Rho Opiuchi Cloud Complex Nearest Star-Forming Region Stellar Processes Hydrogen and Helium Stellar Clusters Ongoing Star Formation Protostellar Jets Extreme Environments Galactic Center Massive Planets Cloud Collapse Theories Failed Stars Rho Ophiuchi Supernovas Galaxies Stellar Birth Nebula Starburst Patterns Large Magellanic Cloud Dusty Clouds Galaxy Formation Early Phase Cosmic Forces Acceleration Effects of Ram Pressure Radcliffe Wave Massive Young Stars Early Star Formation Water Vapor Observations Star-Forming Environments Formation Processes Early Stages Planetary Development Radiation Triangulum Galaxy (M33) Herbig-Haro Object First Stars Turbulence Rate Starburst Galaxy Newly Born Stars Protostellar Disk Protostellar Disks Population III Stars Environmental Conditions Galaxy Evolution Galaxy Characteristics Hydrogen Gas Molecular Cloud Lifecycle Star Families Stellar Families Molecular Hydrogen Solar Systems Star-forming Regions Binary Stars Protoplanetary Discs White Dwarfs Dust Disks T Tauri Stars Rosette Nebula 3D Mapping Milky Way Galaxy Star-Forming Galaxies Cosmology
Multiwavelength data show visible dimming with an infrared spike, signaling hot debris from an impact.
