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Is 0716+714 a superluminal blazar?

U. Bach·T. P. Krichbaum·E. Ros·A. Witzel·J. A. Zensus·S. Britzen
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Abstract

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.

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U. Bach, T. P. Krichbaum, E. Ros, A. Witzel, J. A. Zensus, S. Britzen. 2002-07-03. Is 0716+714 a superluminal blazar?. https://arxiv.org/abs/astro-ph/0207083

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