Hostname: page-component-84b7d79bbc-4hvwz Total loading time: 0 Render date: 2024-07-27T23:35:58.896Z Has data issue: false hasContentIssue false
  • English
  • Français

HST and KECK Observations of High Redshift Radio Galaxies

Published online by Cambridge University Press:  25 May 2016

W.J.M. Van Breugel
W.J.M. Van Breugel*
Affiliation:
Institute of Geophysics and Planetary Physics Lawrence Livermore National Laboratory P.O. Box 808, L-413, Livermore, CA 94550, USA

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.

Together with several of my colleagues I have embarked on a comprehensive program to study the radio–aligned restframe UV structures in high redshift radio galaxies (HzRGs) using some of the world's premier optical telescopes: the Hubble Space Telescope for high spatial resolution imaging, and the Keck 10m telescope for high S/N spectropolarimetry. I will discuss some of our latest results from these observations which elucidate, and at the same time obscure, our evolving understanding of HzRGs.

Type
Cosmological Implications
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 577 - 580
Copyright
Copyright © Kluwer 1996