Very High Redshift Radio Galaxies
Astrophysics
2007-05-23 v1
Abstract
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 are selected, the evidence for strong morphological evolution at near-infrared wavelengths, and for jet-induced star formation in the z=3.800 HzRG 4C41.17.
Cite
@article{arxiv.astro-ph/9806135,
title = {Very High Redshift Radio Galaxies},
author = {Wil van Breugel and Carlos De Breuck and Huub Rottgering and George Miley and Adam Stanford},
journal= {arXiv preprint arXiv:astro-ph/9806135},
year = {2007}
}
Comments
10 Pages, including 8 PostScript figures; To appear in "Looking Deep in the Southern Sky" eds R.Morganti & W.J.Couch, Proc. of ESO/Australia Workshop, Dec 97 Sydney