On galaxy morphology in small groups

Details On galaxy morphology in small groups On galaxy morphology in small groups

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246l...5b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 246, May 15, 1981, p. L5-L9.

Astronomy and Astrophysics

Astrophysics

39

Galactic Clusters, Galactic Evolution, Galactic Structure, Spiral Galaxies, Astronomical Catalogs, Density Distribution, Elliptical Galaxies, Magnitude

Scientific paper

A study of the galaxy populations in small groups shows that Dressler's relationship between galaxy type and local galaxy density is continuous from the field galaxies through the small groups to the rich clusters. Regions in groups and clusters of similar density have similar populations of elliptical, S0, and spiral galaxies. The loose groups extend the relationship into the low galaxy density regime.

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