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

• Faraday rotationNarrower topic: Its ionized component rotates polarization and reveals the Galaxy’s magnetic structure.

• Interstellar chemistryNarrower topic: Its gas, dust, radiation, and energetic particles provide the setting for interstellar chemistry.

• Interstellar magnetic fieldNarrower topic: The magnetic field is one component of this multiphase material.

• Interstellar objectNarrower topic: Visitors travel through this material, which can erode or alter their surfaces over time.

• Circumstellar mediumNarrower topic: The surrounding galactic gas sets the external conditions encountered by circumstellar material.

• Lyman seriesNarrower topic: Neutral hydrogen in this medium absorbs ultraviolet Lyman-series light.

• Ring NebulaNarrower topic: The Ring Nebula's ejecta will eventually mix into this material.

• 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.

• Lyman SpitzerNarrower topic: Spitzer's theoretical work helped establish the modern study of matter between stars.

• 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.

• Flocculent spiral galaxyNarrower topic: Its distribution supplies the material from which visible arm segments and young stars form.

• 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.

• Reflection nebulaNarrower topic: Reflection nebulae are visible structures within this larger environment.

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

• Outer spaceBroader topic: It describes what occupies the much larger gaps between stars.

• Pillars of CreationNarrower topic: The pillars are dense structures within the interstellar material of the Eagle Nebula.

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

• Ring galaxyNarrower topic: The ring's gas supply determines where it can form stars and how long it remains visible.

• 2I/BorisovNarrower topic: Borisov traveled through this environment before entering the Solar System, where erosion may have altered its surface.

• Astrophysical fluid dynamicsBroader topic: Its turbulent phases form the material from which stars emerge.

• Astrophysical maserNarrower topic: Astrophysical masers are amplified within particular regions of this galactic material.

• 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.

• H I regionNarrower topic: H I regions are one component of this material between stars.

• Local Interstellar CloudNarrower topic: The cloud is one localized structure within this material between stars.

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

• Rosette NebulaNarrower topic: The nebula is a structured, illuminated part of the Milky Way’s interstellar medium.

• Sagittarius B2Narrower topic: The cloud is a concentrated part of the material circulating through the Milky Way’s interstellar medium.

• Stellar astronomyCompared with: Stars form from this material and return matter to it through winds and explosions.

• GlycolaldehydeNarrower topic: Glycolaldehyde is detected in molecular gas within this environment.

• Kennicutt–Schmidt lawNarrower topic: Its gas inventory supplies the surface density used in the relation.

• Local BubbleNarrower topic: The Local Bubble is a cavity within this broader material.

• Rho Ophiuchi cloud complexNarrower topic: The complex is a dense, structured part of this material between stars.

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

• 1I/ʻOumuamuaNarrower topic: Objects such as ʻOumuamua travel through this medium before encountering a planetary system.

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

• Circumstellar discNarrower topic: Circumstellar discs inherit material from the interstellar clouds that collapse to form stars.

• 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.

• High-velocity cloudNarrower topic: High-velocity clouds are a distinct gas component within the Milky Way’s broader interstellar environment.

• Interplanetary mediumNarrower topic: Interstellar material surrounds the heliosphere and contributes neutral atoms and incoming dust.

• Interstellar cloudNarrower topic: Interstellar clouds are denser concentrations within this broader galactic environment.

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