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Fig. C.1.


Top panel: radial distance of VLBI components from the Gaia position referenced to the nova epoch. Filled blue and empty red dots indicate components in the SE and NW regions, respectively. The shaded regions show the best fit and uncertainty of a r ∝ tp fit to the trend. Bottom panel: linear velocity obtained by deriving the power-law motion, in blue and red for the two sides, respectively.

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