We discuss the near infrared observations obtained for a set of 81 gal
axies in the region of the Perseus-Pisces supercluster. From these, in
conjunction with the 21 cm data of the Arecibo sample, we estimate th
e peculiar velocities via the Tully Fisher relation and the model of t
he local perturbations as derived by Han and Mould. From the data disc
ussed we find that the supercluster main structure is shrinking. To ex
plain the size and velocities observed the model requires, for the sup
ercluster. a mean overdensity of about DELTArho/rho = 9 which correspo
nds to a total mass of 10(16) solar masses to cover an extension of ab
out 100 Mpc.