Linked from

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

• 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.

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

• 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.

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

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

• 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.

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

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

• 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.

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

• 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.

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

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