Fig. 2
Separation from the core for the different VLBI components obtained by Kun et al. (2014) for source 1928+738 using from MOJAVE data (Lister et al. 2009b). We fitted components C1, C6, and C8, which have been ejected by black holes Cg, CS, and BHC6. To check the consistency of the model, we fitted components C7a, C9, and C5, which have been ejected by black holes Cg, CS, and BHC6.
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