We show results from a 7 year VLBI monitoring programme of 3C273 at millimeter wavelengths. We find evidence for component acceleration, motion or rotation of fluid dynamical patterns in the VLBI jet, and evidence for an outburst-ejection relation between Gamma-ray flares and the appearance of new jet components.
@article{arxiv.astro-ph/0103443,
title = {A High-Frequency and Multi-Epoch VLBI Study of 3C 273},
author = {T. P. Krichbaum and D. A. Graham and A. Witzel and J. A. Zensus and A. Greve and M. Grewing and A. Marscher and A. J. Beasley},
journal= {arXiv preprint arXiv:astro-ph/0103443},
year = {2007}
}
Comments
4 pages, 5 figures, to appear in: Particles and Fields in Radio Galaxies, a conference held at Oxford August 3-5, 2000, ASP Conference Series, eds. R.A. Laing and K.M. Blundell, in press