Very high redshift radio galaxies

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High redshift radio galaxies (HzRGs) provide unique targets for the study of the formation and evolution of massive galaxies and galaxy clusters at very high redshifts. We discuss how efficient HzRG samples ae selected, the evidence for strong morphological evolution at near-infracd wavelengths, and for jet-induced star formation in the z = 3 800 HzRG 4C41 17

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13 p.

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van Breugel, W. J. M. December 1, 1997.

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Description

High redshift radio galaxies (HzRGs) provide unique targets for the study of the formation and evolution of massive galaxies and galaxy clusters at very high redshifts. We discuss how efficient HzRG samples ae selected, the evidence for strong morphological evolution at near-infracd wavelengths, and for jet-induced star formation in the z = 3 800 HzRG 4C41 17

Physical Description

13 p.

Notes

OSTI as DE98058841

Other: FDE: PDF; PL:

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  • Looking deep in the southern sky, Sydney (Australia), 9-12 Dec 1997

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  • Other: DE98058841
  • Report No.: UCRL-JC--131174
  • Report No.: CONF-971257--
  • Grant Number: W-7405-ENG-48
  • Office of Scientific & Technical Information Report Number: 657374
  • Archival Resource Key: ark:/67531/metadc702487

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  • December 1, 1997

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  • Sept. 12, 2015, 6:31 a.m.

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  • April 10, 2017, 1:24 p.m.

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van Breugel, W. J. M. Very high redshift radio galaxies, article, December 1, 1997; California. (digital.library.unt.edu/ark:/67531/metadc702487/: accessed September 19, 2017), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.