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1999AJ....117.1967S - Astron. J., 117, 1967-1984 (1999/May-0)
The evolution of cluster radio galaxies from z = 0 to z = 0.8.
STOCKE J.T., PERLMAN E.S., GIOIA I.M. and HARVANEK M.
Abstract (from CDS):
The results of this radio continuum survey differ from those studies that took the opposite approach, in which a radio-loud quasar or FR 2 radio galaxy was used as a target for a rich cluster search. While those studies found numerous FR 2's and quasars in rich clusters at z~(1)/(2), this survey has found only FR 1-type sources. The difference between these two approaches may lie in the density of the intracluster medium (ICM) and the galaxy richness of the clusters in these two samples, with the current sample having the demonstrably denser ICMs and richer galaxy populations.
Abstract Copyright: ∼
Journal keyword(s): Galaxies: Clusters: General - Radio Continuum
Nomenclature: Table 2: [SPG99] HHMM+DD A, [SPG99] HHMM+DD AN, N=43.
Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.
CDS comments: Table 1 : 1E 1426.4+1058 misprint for 1E 1426.4+0158. Page 1978 : WAT source 1919+479 is 4C 47.51
Simbad objects: 27
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