Is 0716+714 a superluminal blazar?
| dc.creator | Bach, U. | |
| dc.creator | Krichbaum, T. P. | |
| dc.creator | Ros, E. | |
| dc.creator | Witzel, A. | |
| dc.creator | Zensus, J. A. | |
| dc.creator | Britzen, S. | |
| dc.date | 2002-07-03 | |
| dc.date.accessioned | 2026-07-07T02:04:10Z | |
| dc.date.available | 2026-07-07T02:04:10Z | |
| dc.description | We present an analysis of new and old high frequency VLBI data collected during the last 10 years at 5--22 GHz. For the jet components in the mas-VLBI jet, two component identifications are possible. One of them with quasi-stationary components oscillating about their mean positions. Another identification scheme, which formally gives the better expansion fit, yields motion with $\sim 9$ $c$ for $H_0=65$ km s$^{-1}$ Mpc$^{-1}$ and $q_0=0.5$. This model would be in better agreement with the observed rapid IDV and the expected high Lorentz-factor, deduced from IDV. | |
| dc.description | 2 pages, 3 figures, appears in: Proceedings of the 6th European VLBI Network Symposium held on June 25th-28th in Bonn, Germany. Edited by: E. Ros, R.W. Porcas, A.P. Lobanov, and J.A. Zensus | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0207083 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0207083 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4647 | |
| dc.subject | Astrophysics | |
| dc.title | Is 0716+714 a superluminal blazar? | |
| dc.type | text |