Radio evidence for evolution of galaxies in rich clusters
| 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.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.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.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 |