  We present a study of high-resolution long-slit spectra of the narrow-line
region (NLR) in NGC 1068 obtained with the Space Telescope Imaging Spectrograph
(STIS) aboard The Hubble Space Telescope (HST). The spectra were retrieved from
the Multimission Archive at Space Telescope (MAST) obtained from two visits and
seven orbits of HST time. We also obtained MERLIN radio maps of the center of
NGC 1068 to examine the dependence of the NLR cloud velocities on the radio
structure. The radial velocities and velocity dispersions of the bright NLR
clouds appear to be unaffected by the radio knots, indicating that the radio
jet is not the principal driving force on the outflowing NLR clouds. However,
the velocities of the fainter NLR clouds are split near knots in the jet,
indicating a possible interaction. Biconical outflow models were generated to
match the data and for comparison to previous models done with lower dispersion
observations. The general trend is an increase in radial velocity roughly
proportional to distance from the nucleus followed by a linear decrease after
roughly 100 parsec similar to that seen in other Seyfert galaxies, indicating
common acceleration/deceleration mechanisms.
