Radio evidence for evolution of galaxies in rich clusters

Owen, F.N.; Morrison, G.; Dwarakanath, K.S.; Ledlow, M.J.; Miller, N.A.

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

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DC Field	Value	Language
dc.contributor.author	Owen, F.N.	-
dc.contributor.author	Morrison, G.	-
dc.contributor.author	Dwarakanath, K.S.	-
dc.contributor.author	Ledlow, M.J.	-
dc.contributor.author	Miller, N.A.	-
dc.date.accessioned	2007-05-29T10:56:46Z	-
dc.date.available	2007-05-29T10:56:46Z	-
dc.date.issued	2001	-
dc.identifier.citation	ASP Conference Series, 2001, Vol.240, p607	en
dc.identifier.isbn	1-58381-077-3	-
dc.identifier.uri	http://hdl.handle.net/2289/2531	-
dc.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	en
dc.description.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.	en
dc.format.extent	344973 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2001ASPC..240..607O	en
dc.rights	2001 Astronomical Society of the Pacific	en
dc.title	Radio evidence for evolution of galaxies in rich clusters	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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