  A survey of 30 nearby M6.0-M7.5 dwarfs with Ks<12 mag utilizing the Hokupa'a
adaptive optics system at the Gemini North Telescope has discovered 3 new
binary systems. All 3 systems have separations between 0.12-0.29 arcsec (3-10
AU) with similar mass ratios (q>0.8, Delta Ks<0.7). This result gives further
support to the suggestion that wide (a>20 AU) very low mass (M_{tot}<0.185
M_sun) binary systems are exceedingly rare or perhaps even non-existant. The
semimajor axis distribution of these systems peaks at ~5 AU, tighter than more
massive M and G binary distributions which have a broad peak at separations of
\~30 AU. We find a sensitivity-corrected binary fraction in the range of
5_{-2}^{+4}% for M6.0-M7.5 stars with separations a>3 AU. This binary frequency
is less than the ~32% measured among early M dwarfs over the same separation
range. Two of the low-mass binaries are probable Hyades open cluster members
based on proper motions, cluster membership probabilities, radial velocities,
and near-IR photometry. LP415-20 has the distinction of being the tightest (3.6
AU) multiple system ever spatially resolved in the cluster and the companions
of LP415-20 and LP475-855 are among the least massive objects ever resolved in
the Hyades with estimated masses of 0.081_{-0.010}^{+0.009} and
0.082_{-0.009}^{+0.009} M_{\sun}.
