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We present radial velocities for approximately 40 stars in each of threeoptically obscured, off-axis, fields toward the Galactic bulge. Combined withthe data presented by Blum et al. (1994), we now have mean radial velocitiesand radial velocity dispersions in four fields towards the Galactic bulge.These four fields lie nearly along an axis whose position angle from the majoraxis of the Galaxy is 55\deg. The observed kinematics generally match bothKent's (1992) axisymmetric and Zhao's (1994) barred dynamical modelpredictions, but are marginally better described by the latter. The velocitydispersion in our innermost field is high, 153 $\pm$ 17 \kms. Our data,combined with that from previous studies at larger radii, suggest that thestellar velocity dispersion is flat or still rising at projected radius R \aple150 pc.Comment: 31 pages, 5 figures, uuencoded postscript. Accepted for publication  in the Astrophysical Journal

M Giant Kinematics in Off-Axis Fields between 150 and 300 Parsecs from the Galactic Center