A Sharper View into the Parsec-Scale Jet of 3C345

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Scientific paper

We present images from VSOP observations of 3C345 at 6cm, for two epochs separated by 1 year. In the VSOP images, the inner jet of 3C345 is resolved into several components, which cannot be disentangled from each other in the ground VLBI images. The components show superluminal motions, with different trajectories and large variations in the flux densities. These observations help us to obtain better constrains for the models of 3C345.

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