Linked from

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

• Star formationNarrower topic: Star formation transforms dense portions of this galactic material into stars.

• Molecular cloudNarrower topic: Molecular clouds are its cold, dense component.

• Stellar windNarrower topic: Stellar winds inject material and energy into this galactic environment.

• Protoplanetary diskNarrower topic: A young star and its disk form from collapsing interstellar material.

• H II regionNarrower topic: H II regions are structured parts of this broader material.

• Solar windNarrower topic: The solar wind eventually meets this surrounding material at the heliosphere’s outer boundary.

• Interstellar dustNarrower topic: Interstellar dust is the solid component of this broader galactic environment.

• Interstellar extinctionNarrower topic: Extinction research emerged from recognizing this material as an active influence on starlight.

• Stellar feedbackNarrower topic: It is the material into which stellar feedback deposits energy and matter.

• Voyager 1Narrower topic: Voyager 1's instruments now measure particles and fields in this environment beyond the heliopause.

• Asymptotic giant branchNarrower topic: Ejected branch-star material returns processed elements and dust to this medium.

• Molecular hydrogenNarrower topic: Molecular hydrogen forms and persists within this broader material between stars.

• Galactic diskNarrower topic: The disk contains much of a galaxy’s cold, star-forming interstellar material.

• Planet formationNarrower topic: Its material supplies the raw ingredients inherited by planet-forming disks.

• Solar nebulaNarrower topic: The solar nebula formed from material drawn from this larger galactic reservoir.

• Emission nebulaNarrower topic: An emission nebula is a bright, ionized structure within this broader material.

• Galactic CenterNarrower topic: Its gas and dust shape the material and visibility of the central environment.

• Herbig–Haro objectNarrower topic: Jet collisions with this surrounding material generate the nebular emission.

• NebulaNarrower topic: Nebulae are denser regions within this diffuse galactic material.

• Galactic windNarrower topic: It supplies much of the material swept up and heated by galactic winds.

• Herschel Space ObservatoryNarrower topic: Herschel surveyed its cold components, which provide the raw material for stellar systems.

• Nebular hypothesisNarrower topic: The Solar System's precursor cloud was part of this broader material environment.

• AstrochemistryNarrower topic: Its diffuse gas and dust provide the setting for much astrochemical activity.

• Dispersion measureNarrower topic: Its free electrons contribute to the Galactic portion of a measured dispersion measure.

• Carbon starNarrower topic: Carbon-star winds return nucleosynthesis products to the material from which future stars form.

• Cassiopeia ANarrower topic: Cassiopeia A’s expanding shock sweeps up and heats this surrounding material.

• Circumstellar envelopeNarrower topic: An expanding envelope eventually mixes into the surrounding interstellar medium.

• Cosmic dustNarrower topic: Cosmic dust is a small but consequential solid component of this material.

• Dark nebulaNarrower topic: Dark nebulae are dense structures embedded in this galactic material.

• 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.

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

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

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

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

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

• 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.

• 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.

• 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.