Polarimetry of powerful radio galaxies from z=0 to z=4
| dc.creator | Tadhunter, Clive | |
| dc.date | 2005-01-19 | |
| dc.date.accessioned | 2026-07-07T02:16:47Z | |
| dc.date.available | 2026-07-07T02:16:47Z | |
| dc.description | The advent of sensitive polarimeters on large telescopes has led to a revolution in our understanding of active galaxies over the last 20 years. In the case of powerful radio galaxies the deep polarimetric measurements made possible by the new technology have: (a) provided the most direct evidence to support the unified schemes for powerful radio galaxies; (b) enhanced our understanding of the colours and morphologies of radio source host galaxies at all redshifts; and (c) provided key information about the kinematics and geometries of the scattering regions on a sub-kpc scale. | |
| dc.description | 12 pages, 3 figures Invited review article to appear in the proceedings of the Astronomical Polarimetry 2004 Conference, Waikaloa, Hawaii | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0501408 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0501408 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8923 | |
| dc.subject | Astrophysics | |
| dc.title | Polarimetry of powerful radio galaxies from z=0 to z=4 | |
| dc.type | text |