FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters

Details FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters

1999-10-06

arxiv.org/abs/astro-ph/9910099v1

Astronomy and Astrophysics

Astrophysics

42 pages, including 15 figures (10 as separate jpeg files) and 6 tables; accepted to ApJ

Scientific paper

10.1086/308428

Bent-double radio sources can act as tracers for clusters of galaxies. We present imaging and spectroscopic observations of the environments surrounding ten of these sources (most of them Wide Angle Tails (WATs)) selected from the VLA FIRST survey. Our results reveal a previously unknown cluster associated with eight of the radio sources with redshifts in the range 0.33 < z < 0.85; furthermore, we cannot rule out that the other two bent doubles may be associated with clusters at higher redshift. Richness measurements indicate that these clusters are typical of the majority of those found in the Abell (1958) catalog, with a range of Abell richness classes from 0 to 2. The line-of-sight velocity dispersions are very different from cluster to cluster, ranging from approximately 300 to 1100 km/s. At the upper end of these intervals, we may be sampling some of the highest-redshift massive clusters known. Alternatively, the large velocity dispersions measured in some of the clusters may indicate that they are merging systems with significant substructure, consistent with recent ideas concerning WAT formation (Burns et al. 1994).

Affiliated with

Also associated with

No associations

Rating

FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-528502