Fig. 6.
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Comparison of the rotation rate of the polarization angle rotation event at 10.45 GHz shown in Myserlis et al. (2018) and the rotation rate of the helical jet shape along the jet direction as seen in the 2016 RadioAstron observations of OJ 287. In both cases we see a tighter winding of the jet helical, with it bending closer to the jet base.
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