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.

• 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.

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

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

• 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.

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

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

• 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.