morphology
(form and structure)
The English word, morphology, refers to the form and structure
of something, and in astrophysics, the word is often used for
extended sources, perhaps most often for galaxies.
The word is used in descriptions and in classification terms that
are specifically not based upon function or dynamics, but rather
the shape and appearance of the object.
The Hubble classification of galaxies is termed
a morphological classification.
The term also can be used for protoplanetary disks, planetary nebulae,
supernova remnants and other clouds, as well as stellar clusters,
galaxy clusters, and planets and asteroids.
(galaxies,terminology)
Further reading:
https://en.wikipedia.org/wiki/Galaxy_morphological_classification
https://en.wiktionary.org/wiki/morphology
https://dictionary.obspm.fr/index.php?showAll=1&formSearchTextfield=morphology
https://astronomy.swin.edu.au/cosmos/g/Galaxy+Morphology
Referenced by pages:
bar
Bautz-Morgan classification
Catalog of Galaxies and Clusters of Galaxies (CGCG)
galaxy
galaxy classification
galaxy formation
Gini/M20
Magellanic Clouds (MC)
Morgan classification
Morphological Catalogue of Galaxies (MCG)
morphology-density relation
PCA analysis
peculiar galaxy (p)
principal component analysis (PCA)
Radio Galaxy Zoo (RGZ)
van den Bergh galaxy classification
Index