Linked from

The 26 pages that link to Galaxy morphology, each with the reason it gives.

• Galaxy evolutionRelated: Structural transformation is one visible outcome of galaxy evolution.

• Weak gravitational lensingRelated: Lensing measurements must estimate and correct the intrinsic shapes of source galaxies.

• Hierarchical structure formationRelated: Mergers can transform disks into spheroids and reshape stellar distributions.

• Galaxy interactionRelated: Mergers can transform orderly disks into more spheroidal remnants.

• Galaxy harassmentRelated: Changes in disks, bars, and bulges provide evidence for structural transformation.

• Optical astronomyRelated: Optical images show the structures used to classify galaxies and study their evolution.

• Hubble Ultra-Deep FieldRelated: Resolved sources offer examples for tracing how galaxy structure changes with distance.

• Extragalactic astronomyRelated: Morphology provides a basic way to compare galaxy types and their evolution.

• Field galaxyRelated: Comparing field and cluster morphologies tests how environment changes galaxy structure.

• Galactic astronomyRelated: The Milky Way’s precise spiral pattern and bar geometry remain difficult to map from within.

• Interacting galaxyRelated: Tidal distortions can change the forms used to classify galaxies.