Linked from

The 111 pages that link to Interstellar medium, each with the reason it gives.

• Stellar nucleosynthesisRelated: Stellar winds and explosions return synthesized elements to this material.

• MetallicityRelated: It receives stellar ejecta and supplies chemically enriched material for later generations of stars.

• Supernova remnantRelated: Its density and composition shape the remnant’s expansion and appearance.

• Planetary nebulaRelated: The expanding shell eventually mixes into its surrounding galactic environment.

• Elliptical galaxyRelated: Its relative scarcity helps explain why most ellipticals form few new stars.

• Galaxy evolutionRelated: Its phases supply star-forming material and respond to feedback.

• Galaxy formation and evolutionRelated: Its phases exchange material as stars form, evolve, and return gas.

• Voyager programRelated: Voyager instruments now sample plasma and particles in this region beyond the heliopause.

• Ultraviolet astronomyRelated: Ultraviolet absorption lines trace its composition, temperature, and structure.

• Galactic bulgeRelated: Its material can accumulate in bulges and fuel star formation or central activity.

• HeliosphereRelated: Its pressure and magnetic field interact with the solar wind at the heliopause.

• Galactic chemical evolutionRelated: It receives stellar ejecta and supplies material for later generations of stars.

• Dwarf galaxyRelated: Its presence or loss helps separate gas-rich irregular dwarfs from gas-poor spheroidals.

• Galactic coordinate systemRelated: Its disk-wide distribution is often mapped against Galactic longitude and latitude.

• Spiral armRelated: Its clouds and dust lanes trace material concentrated in spiral arms.

• Irregular galaxyRelated: Its clouds provide the material for the vigorous star formation seen in many irregulars.

• Magellanic CloudsRelated: Their abundant gas supplies material for ongoing star formation.

• Stellar metallicityRelated: Its enrichment sets the material from which stars inherit their initial composition.

• Triangulum GalaxyRelated: Its gas supplies the material from which M33 continues to form stars.

• Galactic barRelated: Gas in the interstellar medium responds to the bar’s gravitational potential.

• Interstellar travelRelated: At high spacecraft speeds, even thin interstellar matter can create damaging impacts and drag.

• MiraRelated: Mira returns ejected material to the surrounding interstellar environment.

• ProtiumRelated: Protium occurs in atomic and molecular hydrogen throughout interstellar gas.

• Cartwheel GalaxyRelated: The Cartwheel’s ring compresses interstellar gas into sites of new star formation.

• Cat's Eye NebulaRelated: The nebula's outer material eventually expands into the surrounding interstellar environment.

• HeliopauseRelated: Its resistance to the solar wind underlies the predicted boundary.

• Messier 51Related: Its distribution and compression can be studied across the Whirlpool’s arms and interaction features.

• Presolar grainRelated: Condensed grains traveled through interstellar space before entering the solar birth cloud.

• Astronomical objectRelated: It supplies material to some objects and is altered by others.

• Richard SmalleyRelated: Kroto studied carbon-chain molecules detected in this environment before the fullerene experiment.

• Bondi accretionRelated: Its density and temperature set the ambient conditions for possible Bondi-like capture.

• Galactic planeRelated: Much of the Milky Way’s interstellar material lies close to its plane.

• Orion ArmRelated: Its concentrations trace the material associated with spiral arms.

• Space physicsRelated: Its interaction with the heliosphere's boundary remains a frontier for in-situ measurements.

• Andromeda–Milky Way collisionRelated: Gas clouds can collide and be compressed even though individual stars are widely separated.

• Galactic astronomyRelated: Its clouds supply material for new stars and trace the Galaxy’s structure.

• HeliophysicsRelated: Its pressure and magnetic field shape the heliosphere’s outer boundary.

• NGC 5548Related: Gas along the line of sight can absorb and reshape radiation from NGC 5548’s nucleus.

• NGC 6946Related: Its gas fuels new stars, while its dust can obscure supernova light.

• Scutum–Centaurus ArmRelated: Its dense clouds trace much of the arm’s structure.

• Sulfur monoxideRelated: SO's astronomical detections trace sulfur chemistry in this diffuse material.

• Cygnus LoopRelated: The remnant’s expanding shock heats and compresses this surrounding material.

• Formation and evolution of stars and galaxiesRelated: Its changing composition and structure regulate the material available for new stars.

• Zeta OphiuchiRelated: Material in this medium is swept up and heated around the moving star.