The Radio Population in Rich z 0.2 Abell Clusters

Details The Radio Population in Rich z 0.2 Abell Clusters The Radio Population in Rich z 0.2 Abell Clusters

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.1013r&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #10.13; Bulletin of the American Astronomical Society, Vol. 31, p.1390

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a detailed, multi-wavelength analysis of an X-ray bright sample of rich Abell clusters at z 0.2. Specifically, we examine the cluster-wide radio population at luminosities reaching down to low level AGN and star formation driven systems. In general, these clusters contain a relatively high fraction of radio galaxies, some with a significant number of low luminosity sources. The radio population is analyzed in the context of the galaxy colors and spatial distribution and the large and small scale X-ray environment. Preliminary results indicate that the radio population is linked to the dynamical state of the cluster and the large scale environment in which it resides.

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