Linked from

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

• Galaxy mergerNarrower topic: Merger-induced changes in disks, bars, and tails are tracked through morphology.

• Elliptical galaxyNarrower topic: Elliptical galaxies are one major form in the classification of galaxy shapes.

• 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.

• Hubble sequenceNarrower topic: This broader descriptive framework supplies the traits used to classify galaxies.

• Barred spiral galaxyNarrower topic: Bar presence, arm form, and central bulge are key morphological traits.

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

• Lenticular galaxyNarrower topic: Lenticular galaxies occupy a distinct class in the system that organizes galaxy shapes.

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

• Dwarf galaxyNarrower topic: Dwarf galaxies include several distinct shapes rather than one uniform form.

• 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.

• Irregular galaxyNarrower topic: Irregularity is one morphological description among several distinct galaxy forms.

• Galaxy ZooNarrower topic: The project turns visual judgments about galaxy morphology into a large research dataset.

• Grand-design spiral galaxyNarrower topic: Arm coherence is one morphological feature used to describe spiral galaxies.

• Flocculent spiral galaxyNarrower topic: Flocculent spirals are defined by morphology rather than a unique formation mechanism.

• Hoag's ObjectNarrower topic: Its unusually symmetric form challenges ordinary visual classifications of galaxies.

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

• Dwarf elliptical galaxyNarrower topic: Morphology distinguishes dwarf ellipticals from disks and diffuse dwarf spheroidals.

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

• Peculiar galaxyNarrower topic: Peculiarity is often defined by departure from familiar morphological patterns.

• 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.

• Unbarred spiral galaxyNarrower topic: Morphological schemes distinguish spirals with bars from those without them.

• de Vaucouleurs's lawNarrower topic: The law grew from efforts to quantify galaxy structure.