Linked from

The 48 pages that link to Galaxy formation and evolution, each with the reason it gives.

• James Webb Space TelescopeRelated: Deep Webb observations reveal galaxies at different stages of early evolution.

• Cosmic webRelated: Galaxies form within halos supplied by matter flowing along the web.

• N-body simulationRelated: Gravitational simulations model how dark matter halos grow and merge around galaxies.

• Galactic bulgeRelated: Bulges record processes that built and reshaped galaxies.

• Galaxy groupRelated: Group environments alter galaxy histories through interactions and shared gas.

• Galaxy luminosity functionRelated: Predicted galaxy counts by brightness provide a test of how galaxies form and evolve.

• Thirty Meter TelescopeRelated: The telescope’s light-gathering power would support studies of distant galaxies across cosmic history.

• Lookback timeRelated: Different lookback times reveal galaxies at different stages of their development.

• Vera RubinRelated: Dark matter inferred from rotation curves became central to models of how galaxies assemble.

• Local VoidRelated: Sparse galaxy formation within underdense regions makes the Local Void appear especially empty.

• Neil deGrasse TysonRelated: It is among the astrophysical subjects connected to Tyson’s research and public explanations.

• Gemini ObservatoryRelated: Gemini spectroscopy helps measure distant galaxies’ properties and evolutionary stages.

• Universe (cosmology)Related: Galaxies are major structures built during cosmic evolution.

• Extragalactic astronomyRelated: Comparing galaxies across cosmic time tests models of their life histories.

• Giant Magellan TelescopeRelated: The telescope’s light-gathering power is intended to probe faint, distant galaxies.

• Chronology of the universeRelated: It describes how early density fluctuations became the galaxies seen in later cosmic eras.

• Lyman-alpha emitterRelated: Emitter populations reveal how young galaxies build stars and acquire gas.

• Astronomical black holesRelated: Supermassive black holes can influence star formation and gas flows in their host galaxies.

• Computational astrophysicsRelated: Simulations trace how gravity, gas cooling, and stellar feedback build galaxies.

• de Vaucouleurs's lawRelated: Profile shape and scale help compare galaxy structures across populations and epochs.

• Infrared telescopeRelated: Infrared surveys test models of how galaxies grew during the universe's first billion years.