  The cosmic microwave background (CMB) is a unique probe of cosmological
parameters and conditions. There is a connection between anisotropy in the CMB
and the topology of the Universe. Adopting a universe with the topology of a
3-Torus, or a universe where only harmonics of the fundamental mode are
allowed, and using 2-years of COBE/DMR data, we obtain constraints on the
topology of the Universe. Previous work constrained the topology using the
slope information and the correlation function of the CMB. We obtain more
accurate results by using all multipole moments, avoiding approximations by
computing their full covariance matrix. We obtain the best fit for a cubic
toroidal universe of scale 7200h^{-1} Mpc for n=1. The data set a lower limit
on the cell size of 4320h^{-1} Mpc at 95% confidence and 5880h^{-1} Mpc at 68%
confidence. These results show that the most probable cell size would be around
1.2 times larger than the horizon scale, implying that the 3-Torus topology is
no longer an interesting cosmological model.
