Hostname: page-component-7c8c6479df-27gpq Total loading time: 0 Render date: 2024-03-29T04:43:07.540Z Has data issue: false hasContentIssue false

The properties of galaxies on the outskirts of clusters

Published online by Cambridge University Press:  06 October 2004

Erica Ellingson
Affiliation:
Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309, USA email: elling@casa.colorado.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The outskirts of clusters are dynamically complex regions populated by galaxies falling into the cluster potential for the first time as well as some which have already visited the cluster core. Addressing the properties of galaxies in these transition regions requires the integration of cluster dynamics, an understanding of environmental influences on galaxies at both high and low densities and hierarchical scenarios of cluster formation and growth. In this review I describe some recent observational results on galaxies in the outskirts of clusters, and the evolution of galaxies in clusters as a function of local density and radius.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union