  The EFAR project has measured peculiar motions in two distant volumes of the
universe using Fundamental Plane (FP) distances for 85 clusters with
cz=6000-15000 km/s. The scatter in distance about the FP is observed to be 20%
per galaxy for EFAR sample, resulting in peculiar velocities with a median
precision of 1075 km/s for the 50 clusters with 3 or more galaxies. We find
that there is no evidence for a large bulk flow within either of the two
volumes sampled by the EFAR clusters. The measured bulk motion in both regions
is small and consistent with zero. The Lauer and Postman (1994) bulk motion is
ruled out at the 4-sigma level. There is no evidence supporting the SMAC
(Hudson et al. 1999) or LP10K (Willick 1999) bulk motions, but the
directionality of the EFAR sample would only allow a weak (2-sigma) detection
at best.
