Lists of (member) stars used to derive the astrometric parameters for each object:
Without annotations:
Without orbits/arcs:
Velocity fields derived from proper motions for the Magellanic Clouds:
The second movie shows that two dwarfs (Ursa Minor and Draco) share very similar orbits and that many of the dwarfs, but not all, lie in a common fairly planar configuration.
These movies are created with ipyvolume
