  We consider the possibility that the Galactic neutral hydrogen stream Complex
A and the stellar Orphan stream are related, and use this hypothesis to
determine possible distances to Complex A and the Orphan stream, and
line-of-sight velocities for the latter. The method presented uses our current
knowledge of the projected positions of the streams, as well as line-of-sight
velocities for Complex A, and we show that a solution exists in which the two
streams share the same orbit. If Complex A and the Orphan stream are on this
orbit, our calculations suggest the Orphan stream to be at an average distance
of 20 kpc, with heliocentric radial velocities of approximately -110 km/s.
Complex A would be ahead of the Orphan stream in the same wrap of the orbit,
with an average distance of 10 kpc, which is consistent with the distance
constraints determined through interstellar absorption line techniques.
