The Early History of Powerful Radio Galaxies
| dc.creator | Dey, Arjun | |
| dc.date | 1998-02-12 | |
| dc.date.accessioned | 2026-07-07T02:26:04Z | |
| dc.date.available | 2026-07-07T02:26:04Z | |
| dc.description | I briefly review the current status of observations of AGN-powered UV/optical light, starlight, dust and outflow phenomena in high-redshift powerful radio galaxies. The existing data are consistent with the hypothesis that powerful radio galaxies undergo a major episode of star formation at high redshift z>4 during which they form most of their stars, and subsequently evolve `passively', with the UV continuum emission in the z~1 galaxies being dominated by AGN-related processes rather than starlight from the underlying, aging population. | |
| dc.description | 14 pages, to appear in the proceedings of the KNAW colloquium ``The Most Distant Radio Galaxies'' held in Amsterdam on 15-17 October 1997 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9802163 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9802163 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12126 | |
| dc.subject | Astrophysics | |
| dc.title | The Early History of Powerful Radio Galaxies | |
| dc.type | text |