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The morphology-density relation - The group connection

Postman, M., Geller, M. J.·1984·The Astrophysical Journal

Abstract

The relationship between galaxy morphology and local density is derived from two complete galaxy redshift surveys. This relationship is completely consistent with the one derived by Dressler for a sample of 55 rich clusters. The apparently universal morphology-density relation extends over six orders of magnitude in galaxy space density. There is no dependence of galaxy morphology on density in regions where the dynamical time scale is comparable with or greater than the Hubble time. At densities greater than about 600 galaxies/cu Mpc, S0's dominate the galaxy population. At these densities, stripping mechanisms are likely to affect the galaxy population. At densities greater than about 3000 galaxies/cu Mpc, the fraction of elliptical galaxies rises steeply. In these regions, the collapse time is short compared with typical time scales for the formation of disks.

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Metadata

Authors
Postman, M., & Geller, M. J.
Venue
The Astrophysical Journal
Published
1984-06
Volume
281
Pages
95
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2002569490
Cited by
646
References
0
FWCI
6.52
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The morphology-density relation - The group connection. https://app.cochat.ai/papers/10.1086/162078
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Postman, M., & Geller, M. J. (1984). The morphology-density relation - The group connection. The Astrophysical Journal. https://doi.org/10.1086/162078

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