KnowraStar formationLinked fromLinked fromThe 95 pages that link to Star formation, each with the reason it gives.All 95Broader topic 2Related 63Narrower topic 30Field galaxyRelated: Relatively undisturbed gas reservoirs can sustain star formation in many field galaxies.Galactic astronomyRelated: Mapping young stars reveals where the Milky Way is actively building new stellar populations.GALEXRelated: Ultraviolet light from young massive stars let GALEX estimate recent star formation in galaxies.High-velocity cloudRelated: Cloud infall can replenish the disk’s gas reservoir and thereby sustain future star formation.Interstellar cloudRelated: Cloud collapse supplies the material from which new stars form.NGC 6946Related: Its active star formation produces massive stars that later explode as supernovae.Scutum–Centaurus ArmRelated: The arm’s gas-rich regions host sites where new stars form.Edwin E. SalpeterRelated: The initial mass function links the process of star formation to the masses of its stellar products.Infrared telescopeRelated: Infrared telescopes expose embedded protostars hidden from visible-light observatories.List of interstellar and circumstellar moleculesRelated: Molecular tracers map the cold gas from which stars form.Magellanic spiralRelated: Bright star-forming regions can make loosely organized arms conspicuous in these galaxies.Submillimetre astronomyRelated: Cold dust and molecular gas around forming stars emit strongly at submillimetre wavelengths.Viktor AmbartsumianRelated: Ambartsumian argued that stellar associations showed star formation was ongoing.Previous2 of 2