Very High Redshift Radio Galaxies

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dc.creatorvan Breugel, Wil
dc.creatorDe Breuck, Carlos
dc.creatorRottgering, Huub
dc.creatorMiley, George
dc.creatorStanford, Adam
dc.date1998-06-10
dc.date.accessioned2026-07-07T02:27:10Z
dc.date.available2026-07-07T02:27:10Z
dc.descriptionHigh 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.
dc.description10 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9806135
dc.identifierhttp://arxiv.org/abs/astro-ph/9806135
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12574
dc.subjectAstrophysics
dc.titleVery High Redshift Radio Galaxies
dc.typetext

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