Fig. 3

Two trajectory families associated with the VLBI components ejected by CS and the VLBI components ejected by Cg. The two families separate clearly after 1 mas. Components C1 and C9 have been ejected by CS and components C2, C4b, and C11b probably by CS. They form the first VLBI trajectory family. Components C8 and C7a have been ejected by Cg, and components C3, C4a, C10 and C11a probably by Cg. They form the second VLBI trajectory family. The VLBI coordinates are taken from Kun et al. (2014).
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