Linked from

The 29 pages that link to Galaxy evolution, each with the reason it gives.

• GalaxyRelated: Star formation, accretion, and interactions continually reshape galaxies.

• Spiral galaxyNarrower topic: Gas loss, star formation, and interactions can alter a spiral galaxy’s appearance and future.

• Galaxy morphologyRelated: Morphological populations reveal how galaxy structures change across cosmic history.

• Hubble sequenceCompared with: The sequence is morphological, not a proven timeline of galaxy development.

• Radio galaxyNarrower topic: Jet-driven heating can alter the supply of cold gas and affect a massive galaxy’s growth.

• Margaret BurbidgeRelated: Her research on galaxies connected their observed properties with cosmic history.

• Cosmic star-formation historyNarrower topic: The global history provides a benchmark for models of evolving galaxies.

• Galactic windNarrower topic: Winds regulate star formation and redistribute the material galaxies need to grow.

• Galaxy harassmentNarrower topic: Harassment is one proposed environmental pathway within the broader history of galaxies.

• Color indexNarrower topic: Galaxy colors provide evidence about stellar populations and recent star formation.

• Galaxy luminosity functionRelated: Comparing luminosity functions across epochs reveals how galaxy populations change.

• Euclid (space telescope)Related: Euclid's large samples reveal how galaxy populations and clustering change across the universe.

• Galaxy filamentNarrower topic: A galaxy's position in a filament can shape its supply of fuel and its interactions.

• Galaxy ZooRelated: The project's morphology data help investigate how galaxy structure relates to evolutionary history.

• Star formation efficiencyNarrower topic: Galaxy-scale efficiency helps explain how gas supply becomes accumulated stellar mass.

• Extremely Large TelescopeRelated: ELT observations will measure distant galaxies’ properties and formation histories.

• Large Binocular TelescopeRelated: Its large mirrors collect light from distant galaxies used to study their development.

• Square Kilometre ArrayRelated: Large radio surveys can reveal star formation, gas, and magnetic activity across galaxy populations.

• Arp 220Narrower topic: Arp 220 captures a short-lived transformation from interacting galaxies toward a settled remnant.

• Galaxy morphological classificationNarrower topic: The historical tuning-fork diagram was once interpreted as evolution, a view not supported by its shape alone.

• Subaru TelescopeRelated: Subaru surveys trace galaxies across distance to study their development.

• Faber–Jackson relationNarrower topic: Changes in its slope or scatter can reveal how elliptical galaxies formed and evolved.

• Kennicutt–Schmidt lawNarrower topic: The relation helps connect gas reservoirs to a galaxy’s evolving stellar population.

• Peculiar galaxyNarrower topic: Peculiar systems expose episodes of transformation that regular galaxies may conceal.

• Field galaxyNarrower topic: Field galaxies provide evidence about evolution without the strongest cluster-specific influences.

• GALEXNarrower topic: GALEX surveys tracked how ultraviolet activity varies with galaxy age and environment.

• Interacting galaxyNarrower topic: Interactions are one pathway by which galaxies change their masses, shapes, and star-forming activity.

• Intergalactic starNarrower topic: Intergalactic stars record the stellar material removed as galaxies evolve.

• Low-ionization nuclear emission-line regionRelated: LINER emission helps trace residual nuclear activity and ionized gas in nearby galaxies.