Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990rmxaa..21..136a&link_type=abstract
Revista Mexicana de Astronomia y Astrofisica, 21, 136-140.
Astronomy and Astrophysics
Astronomy
4
Clusters: Galaxies, Radio Sources: General
Scientific paper
We analysed Dixon's Master List of Radio Sources and four large radio surveys for a concentration of sources towards the centres of Abell clusters of galaxies. Using all radio sources, regardless of optical identification, we find that at all frequencies the amount of concentration increases strongly with increasing flux density. The density enhancement of sources within 0.1 Abell radii ranges from 3 to 10 above background for the analysed surveys, but rises to about 20 for all of them, when only strong sources are considered. The richer (R>=2) clusters show the highest concentration of sources above background and generally a broader distribution, while the early Bautz-Morgan types (BM < II) show the narrowest one. Often a source deficiency relative to the survey mean is found in the cluster peripheries.
Andernach Heinz
Andreazza Carmen Maria
No associations
LandOfFree
The Distribution of Radio Sources Towards Rich Clusters of Galaxies 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 The Distribution of Radio Sources Towards Rich Clusters of Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Distribution of Radio Sources Towards Rich Clusters of Galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-843602