arXiv · astro-ph/0501117
Emission line galaxies in clusters
Abstract
At the present epoch, clusters of galaxies are known to be a hostile environment for emission-line galaxies, which are more commonly found in low density regions outside of clusters. In contrast, going to higher redshifts the population of emission-line galaxies in clusters becomes progressively more conspicuous, and large numbers of star-forming late-type galaxies are observed. I present an overview of the observational findings and the theoretical expectations regarding the evolution of emission-line galaxies in dense environments, discussing the properties of these galaxies and the current evidence for environmental influences on their evolution.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
B. M. Poggianti. 2005-01-07. Emission line galaxies in clusters. https://doi.org/10.1007/1-4020-4526-3_6
Cite the original work for its findings. Save a collection to share your selection of sources.