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Optical Polarization of 3C 265

Published online by Cambridge University Press:  25 May 2016

M.H. Cohen
Affiliation:
California Institute of Technology Pasadena, CA 91125 Space Telescope Science Institute Baltimore, MD 21218
H.D. Tran
Affiliation:
California Institute of Technology Pasadena, CA 91125 Space Telescope Science Institute Baltimore, MD 21218
P.M. Ogle
Affiliation:
California Institute of Technology Pasadena, CA 91125 Space Telescope Science Institute Baltimore, MD 21218
R.W. Goodrich
Affiliation:
California Institute of Technology Pasadena, CA 91125 Space Telescope Science Institute Baltimore, MD 21218

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3C 265 is a high-redshift (z=0.811) radio galaxy showing extended emission line regions (EELR) to 50 kpc from the nucleus (McCarthy et al 1995). However, it does not show the alignment effect (McCarthy 1993) that is common in distant galaxies: the EELR is not extended along the radio axis.

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

References

Dey, A. and Spinrad, H. (1996) The Radio Galaxy 3C265 Contains a Hidden Quasar Astroph. J. , in press March 1996.Google Scholar
Fernini, I., Burns, J.O., Bridle, A.H. and Perley, R.A. (1993) Very Large Array Imaging of Five FR II 3CR Radio Galaxies, Astronom. J. , Vol. no. 105, pp. 16901709.Google Scholar
McCarthy, P.J. (1993) High Redshift Radio Galaxies, Ann. Rev. Astron. and Astroph. , Vol. no. 31, pp. 639688.CrossRefGoogle Scholar
McCarthy, P.J., Spinrad, H. and van Breugel, W. (1995) Emission-Line Imaging of 3CR Radio Galaxies. I. Imaging Data, Astroph. J. Supp. , Vol. no. 99, pp. 2766.Google Scholar
Tran, H.D., Cohen, M.H. and Goodrich, R.W. (1995) Keck Spectropolarimetry of the Radio Galaxy 3C 234, Astronom. J. , Vol. no. 110, in press December 1995.Google Scholar
Wills, B.J. et. al. (1995) The Hubble Space Telescope Sample of Radio-Loud Quasars: Ultraviolet Spectra of the First 31 Quaasrs, Astroph. J. , Vol. no. 447, pp. 139158.Google Scholar