Narrow-angle tail radio sources and the distribution of galaxy orbits in Abell clusters

1987 ◽  
Vol 316 ◽  
pp. 113 ◽  
Author(s):  
Christopher P. O'Dea ◽  
Craig L. Sarazin ◽  
Frazer N. Owen
1997 ◽  
Vol 474 (2) ◽  
pp. 580-597 ◽  
Author(s):  
P. L. Gomez ◽  
J. Pinkney ◽  
J. O. Burns ◽  
Q. Wang ◽  
F. N. Owen ◽  
...  

1996 ◽  
Vol 175 ◽  
pp. 238-239
Author(s):  
Michael J. Ledlow ◽  
Frazer N. Owen

From the VLA 20cm survey of ≃ 500 Abell clusters reported by (Ledlow and Owen, 1995), we have obtained optical R-Band CCD observations and optical spectra for 265 radio galaxies. The survey is complete for 20cm flux density greater than 10 mJy within 0.3 corrected Abell radii of the cluster center. All Abell clusters with measured z < 0.09 were surveyed. This statistically complete sample was supplemented by ≃ 200 clusters with 0.09 < z < 0.25 including sources with flux density > 200 mJy. Only 6% of the sample consists of FR II radio sources, the remainder are twin-jets, tailed, or compact sources associated with the FR I class.


2002 ◽  
Vol 12 ◽  
pp. 522-524
Author(s):  
Frazer Owen ◽  
Mike Ledlow ◽  
Jean Eilek

AbstractThe properties of radio sources in and outside of Abell clusters are reviewed. The properties of sources in and out of Abell clusters are shown to be surprisingly similar. However, sources in dense cluster cores do not fit this pattern and, as in Virgo A (M87), have a significant, sometimes dominant input of energy into the “cooling core” environment.


1999 ◽  
Vol 120 (1) ◽  
pp. 147-170 ◽  
Author(s):  
Kevin B. Marvel ◽  
Hemant Shukla ◽  
George Rhee
Keyword(s):  

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