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 ∼9c for H0​=65 km s−1 Mpc−1 and q0​=0.5.
This model would be in better agreement with the observed rapid IDV and the
expected high Lorentz-factor, deduced from IDV.Comment: 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. Zensu