Hostname: page-component-848d4c4894-mwx4w Total loading time: 0 Render date: 2024-07-02T08:59:36.296Z Has data issue: false hasContentIssue false
  • English
  • Français

Optical Properties of High Redshift Radio Galaxies

Published online by Cambridge University Press:  07 August 2017

Patrick J. McCarthy ,
Hyron Spinrad  and
Wil van Breugel
Patrick J. McCarthy
Affiliation:
Department of Astronomy, University of California, Berkeley, CA 94720 U.S.A.
Hyron Spinrad
Affiliation:
Department of Astronomy, University of California, Berkeley, CA 94720 U.S.A.
Wil van Breugel
Affiliation:
Department of Astronomy, University of California, Berkeley, CA 94720 U.S.A.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The 3CR catalogue of extragalactic radio sources is now completely identified for b > 15° and redshifts have been determined for > 98% of them (see Djorgovski et al. 1988 for the latest update). The radio galaxies in this catalogue span the redshift range from 0 to 2.48. This sample provides us with a unique opportunity to examine the optical and radio properties of a complete sample over a look-back time comparable to the Hubble time.

Type
Part 10: Radio Galaxies, Components and Structure
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 543 - 545
Copyright
Copyright © Kluwer 1989 

References

Baldwin, J., Phillips, M. M., and Terlevich, R. 1981, P. A. S. P., 93, 5.CrossRefGoogle Scholar
Baum, S. 1988 , The University of Maryland.Google Scholar
Baum, S. et al. 1988, Ap. J. Suppl., in press.Google Scholar
Baum, S., and Heckman, T. 1988, Ap. J., in press.Google Scholar
Chambers, K. C., Miley, G. K., and van Breugel, W. J. M. 1987, Nature, 329, 604.CrossRefGoogle Scholar
Djorgovski, et al., 1988, A. J., in press.Google Scholar
Le Fèvre, O., Hammer, F, Nottale, L., Mazure, A., and Christian, C. 1988, Ap. J. Lett., 324, L1.Google Scholar
Lilly, S. J., and Longair, M. 1984, M. N. R. A. S., 211, 833.Google Scholar
Lilly, S. J. 1988, Ap. J., in press.Google Scholar
McCarthy, P. J. 1989 , The University of California.Google Scholar
McCarthy, P. J., van Breugel, W. J. M., Spinrad, H., and Djorgovski, S. 1987, Ap. J. Lett., 321, L29.Google Scholar
McCarthy, P. J., et al., 1988, in Cooling Flows in Clusters and Galaxies, Fabian, A. C. ed., Kluwer Academic Publshers, in press. Google Scholar
Spinrad, H. and Djorgovski, S. 1984, P. A. S. P., 96, 795.Google Scholar
Spinrad, H. 1988 in Epoch of Galaxy Formation, Frenk, C. F. ed., Reidel, in press.Google Scholar
Terlevich, R., and Melnick, J. 1985, M. N. R. A. S., 213, 831.CrossRefGoogle Scholar
Unger, S. W. et al. 1987, M. N. R. A. S., 228, 671.Google Scholar
van Breugel, W. J. M. and McCarthy, P. J. 1987, in Proc. Conf. on Active Galactic Nucle, Miller, H. R. and Witta, P. J. eds., Spinger-Verlag.Google Scholar