  We present Tully-Fisher observations for 35 rich Abell clusters of galaxies.
Results from I band photometry and optical rotation curve work comprise the
bulk of this paper. This is the third such data installment of an all-sky
survey of 52 clusters in the distance range 50 to 200\h Mpc. The complete data
set provides the basis for determining an accurate Tully-Fisher template
relation and for estimating the amplitude and direction of the local bulk flow
on a 100\h Mpc scale.
