Radio evidence for evolution of galaxies in rich clusters

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2531

Title:	Radio evidence for evolution of galaxies in rich clusters
Authors:	Owen, F.N. Morrison, G. Dwarakanath, K.S. Ledlow, M.J. Miller, N.A.
Issue Date:	2001
Publisher:	Astronomical Society of the Pacific
Citation:	ASP Conference Series, 2001, Vol.240, p607
Abstract:	We report the status of the radio evidence for the evolution of galaxies in rich clusters for 0.02 < z < 0.41. We find evidence that there has been significant evolution in the star-forming galaxies over this redshift range. No clear evidence is seen for evolution in the radio active galactic nucleus population in clusters over this range. The fraction of galaxies which are radio emitters in rich clusters appears to be enhanced in cluster-cluster mergers.
Description:	Restricted Access. Gas and Galaxy Evolution, ASP Conference Proceedings, Vol. 240. Eds. John E. Hibbard, Michael Rupen, and Jacqueline H. van Gorkom. San Francisco: Astronomical Society of the Pacific, 2001
URI:	http://hdl.handle.net/2289/2531
ISBN:	1-58381-077-3
Alternative Location:	http://adsabs.harvard.edu/cgi-bin/bib_query?2001ASPC..240..607O
Copyright:	2001 Astronomical Society of the Pacific
Appears in Collections:	Research Papers (A&A)

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