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Fig. 15


The kinematic velocity distributions for our sample. The U (top left) and W (bottom left) velocity distributions appear symmetrical around peaks just off zero. Whereas the V (upper right) and total kinematic velocity distribution (lower right) are far from symmetrical. The V distribution shows a fairly high fraction of high proper motion objects moving against the plane of galactic rotation.

This figure is made of several images, please see below:

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