Radio imaging of core-dominated high redshift quasars
| dc.creator | Barthel, Peter D. | |
| dc.creator | Vestergaard, Marianne | |
| dc.creator | Lonsdale, Colin J. | |
| dc.date | 1999-11-25 | |
| dc.date.accessioned | 2026-07-07T02:34:40Z | |
| dc.date.available | 2026-07-07T02:34:40Z | |
| dc.description | VLA imaging at kiloparsec-scale resolution of sixteen core-dominated radio-loud QSOs is presented. Many objects appear to display variable radio emission and their radio morphologies are significantly smaller than those of steep-spectrum quasars, consistent with these objects being observed at sight lines close to their (relativistic, $γ\approx$ 4-7) jet axes. The usefulness of the radio source orientation indicator R_V, being defined as ratio of radio core and rest frame optical V-band luminosity, is confirmed. | |
| dc.description | 11 pages, 11 postscript figures, uses aa.cls 4.03 for LaTeX2e To appear in Astronomy and Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9911474 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9911474 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15332 | |
| dc.subject | Astrophysics | |
| dc.title | Radio imaging of core-dominated high redshift quasars | |
| dc.type | text |