Starting with a general dispersion relation, the three-dimensional rel
ativistic two-body propagator is expressed in terms of relativistic Ja
cobi coordinates. This procedure can be used with most of the widely u
sed propagators. The propagator, written in terms of the Jacobi coordi
nates, is used to define and develop a relativistic two-body wave func
tion. The use of the wave function is illustrated in two cases: photo-
disintegration of a system initially consisting of a bound pair, and t
he calculation of the form factors of such a pair. In each case some m
inimal three body aspects are present. In each case also the connectio
n between the relativistic wave function that we have defined and the
usual nonrelativistic wavefunction based on the Schrodinger equation i
s clearly (and easily) made.