Statistics of spin orientations in binary galaxies may be used as a tool to
study the formation process of galaxies. Helou found that the spins of spi
ral galaxies in binary systems are anticorrelated, and he suggested that it
may have to do with the inclination dependence of the galaxy merger proces
s. We study this dependence in small groups of galaxies. An N-body code is
developed which uses an inclination dependent dynamical friction law to aff
ect mergers of galaxies. It is found that some correlation results in this
way in groups which have initially random spin orientations.