  We analyze rotation velocities and chromospheric (H-alpha) activity, derived
from multi-year, high-resolution spectra, in 56 mid-M to L dwarfs. Rotational
velocities are found to increase from mid-M to L. This is consistent with a
lengthening of spin-down timescale with later type, though in the L types the
trend may also be a function of stellar age. From M5 to M8.5, a saturation-type
rotation-activity relation is seen, similar to that in earlier types. However,
the saturation velocity in our case is much higher, at about 12 km/s. A sharp
drop in activity is observed at about M9, with later types showing little or no
H-alpha emission, in spite of rapid rotation. This may be due to the very high
resistivities in the predominantly neutral atmospheres of these cool objects.
