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.

• Milky WayNarrower topic: The Milky Way’s structure records the general processes that built galaxies in the early universe.

• Globular clusterNarrower topic: Globular clusters trace early episodes in their host galaxies’ assembly.

• Stellar populationNarrower topic: Stellar populations preserve evidence of when and from what material a galaxy formed.

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

• Supermassive black holeNarrower topic: Black-hole feedback is one proposed influence on how galaxies grow and stop forming stars.

• GalaxyBroader topic: It describes how the first galactic systems emerged from early density fluctuations.

• AstronomyBroader topic: Astronomers use galaxy populations to trace the growth of cosmic structure.

• Galaxy morphologyNarrower topic: Formation theories seek to account for the structures that classification records.

• Galaxy rotation curveNarrower topic: Feedback and accretion reshape the mass distributions that curves reveal.

• Stellar feedbackNarrower topic: Feedback regulates gas retention and star formation, shaping galaxies over cosmic time.

• Gravitational instabilityBroader topic: Gravitational growth turns early density variations into galactic structures.

• Hubble sequenceNarrower topic: Formation theories address origins that the Hubble sequence itself does not explain.

• 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.

• Galactic diskNarrower topic: Disk formation is one stage in the broader assembly and evolution of galaxies.

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

• Active galactic nucleus feedbackNarrower topic: Feedback is a major regulator in models of how galaxies acquire and retain gas.

• Cosmic star-formation historyNarrower topic: The cosmic curve summarizes star production across the evolving galaxy population.

• Cosmic infrared backgroundNarrower topic: Evolving galaxies supply the sources whose infrared emission accumulates into the background.

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

• Circumgalactic mediumNarrower topic: The medium regulates the gas supply on which galaxy growth depends.

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

• Intracluster lightNarrower topic: Different galaxy histories predict different contributions to the cluster’s unbound stars.

• 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.

• Hoag's ObjectNarrower topic: Hoag's Object tests whether standard formation pathways explain exceptionally detached rings.

• Hubble Deep FieldNarrower topic: The image's range of galaxy ages and shapes offers evidence about how galaxies changed.

• Hubble Ultra-Deep FieldNarrower topic: The field provides observations of galaxies at many stages of cosmic history.

• Low surface brightness galaxyNarrower topic: Diffuse galaxies constrain how galaxies form and retain or lose their gas.

• 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.

• IC 1101Narrower topic: The exact merger history that produced IC 1101 remains part of broader questions about galaxy growth.

• Structure formationBroader topic: It is the luminous, complex outcome of matter collapsing inside dark-matter halos.

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

• Galactic astronomyNarrower topic: Milky Way history is one nearby case of the broader process of galaxy formation.

• Galaxy rotation problemNarrower topic: Rotation curves constrain models of how galaxies acquire and redistribute mass.

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

• Messier 49Narrower topic: Messier 49’s size and old stars provide evidence about the growth of giant ellipticals.

• 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.

• Sandra FaberNarrower topic: This broad research area frames Faber’s decades of work on how galaxies develop.