Linked from

The 27 pages that link to Ram-pressure stripping, each with the reason it gives.

• Galaxy evolutionRelated: It can quench satellite galaxies through environmental gas loss.

• Galaxy formation and evolutionRelated: It can quench satellites without requiring a major merger.

• Large Magellanic CloudRelated: Motion through the Milky Way’s halo may help strip gas from the Cloud.

• Virgo ClusterRelated: Virgo’s intracluster gas can strip gas from infalling galaxies and suppress star formation.

• Tidal strippingCompared with: It strips gas through hydrodynamic pressure rather than differential gravity.

• Galaxy quenchingRelated: Motion through a dense environment can strip the cold gas needed for star formation.

• Lenticular galaxyRelated: It can deprive a disk galaxy of gas needed to sustain star formation.

• Galaxy groupRelated: A group's hot gas can strip fuel from galaxies moving through it.

• Galaxy interactionCompared with: It can suppress star formation during cluster encounters without requiring another galaxy's gravity.

• Dwarf galaxyRelated: This process can quench star formation in dwarfs inside galaxy groups and clusters.

• Tidal tailCompared with: It can create gas tails without pulling out comparable streams of stars.

• Galactic windCompared with: Unlike feedback-driven winds, this outflow is driven by the galaxy’s motion through external gas.

• Galaxy harassmentCompared with: It can quench star formation in clusters, but acts through gas pressure rather than gravitational encounters.

• Circumgalactic mediumRelated: Dense circumgalactic gas can strip gas from satellite galaxies moving through it.

• Irregular galaxyRelated: It can alter an irregular galaxy’s gas supply and suppress future star formation.

• Magellanic StreamRelated: The Clouds’ motion through the Milky Way’s hot halo pushes gas away and shapes the Stream.

• Satellite galaxyRelated: A satellite crossing its host’s hot halo can lose the gas needed to form stars.

• Fornax ClusterRelated: Fornax galaxies moving through intracluster gas can lose fuel for star formation.

• Magellanic BridgeRelated: It may help shape the Bridge’s gas as the Clouds move through the Milky Way’s halo.

• Dwarf elliptical galaxyRelated: It can deprive an infalling dwarf of gas needed for continued star formation.

• Field galaxyCompared with: The intracluster medium makes this process stronger in clusters than in typical field environments.

• High-velocity cloudRelated: It can strip gas from satellite galaxies, supplying material that becomes high-velocity clouds.

• Interacting galaxyCompared with: It can strip gas without requiring a close gravitational encounter between galaxies.

• Intergalactic starCompared with: It strips gas rather than stars, clarifying which cluster process can liberate intergalactic stars.

• Galaxy groups and clustersRelated: The intracluster medium can strip gas from galaxies and suppress star formation.

• Intergalactic dustRelated: Stripped galactic material can include dust that becomes dispersed between galaxies.

• Starburst regionCompared with: It can suppress star formation by removing fuel, opposite to gas-funneling triggers.