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Optical Properties of FRI Radio Galaxies

Published online by Cambridge University Press:  25 May 2016

Michael J. Ledlow
Affiliation:
Dept. of Astronomy, New Mexico State University Las Cruces, NM 88003-0001, USA National Radio Astronomy Observatory Socorro, NM 87801, USA
Frazer N. Owen
Affiliation:
Dept. of Astronomy, New Mexico State University Las Cruces, NM 88003-0001, USA National Radio Astronomy Observatory Socorro, NM 87801, USA

Extract

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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.

Type
Relation between Radio and Other Wavelenghts
Copyright
Copyright © Kluwer 1996 

References

Auriemma, C.G. et al. 1977, A & A , 57, 41.Google Scholar
Ledlow, M.J. & Owen, F.N. 1995, A J. , 109, 853.CrossRefGoogle Scholar
Sadler, E.M., Jenkins, C.R., & Kotanyi, C.G. 1989, M.N.R.A.S , 240, 591.CrossRefGoogle Scholar