We report the gross properties of the velocity field of the barred spiral galaxy NGC 3367 .
We obtained the following values : inclination with respect to the plane of the sky , i = 30 ; position angle ( P.A . )
of receding semi major axis , P.A . = 51 ^ { \circ } and systemic velocity , V _ { sys } = 3032 km s ^ { -1 } .
Large velocity dispersion are observed of up to 120 km s ^ { -1 } in the nuclear region , of up to 70 km s ^ { -1 } near the eastern bright sources just beyond the edge of the stellar bar where three spiral arms seem to start and in the western bright sources at about 10 kpc .
Deviations from normal circular velocities are observed from all the disk but mainly from the semi circle formed by the string of south western H \alpha sources .
An estimate of the dynamical mass is M _ { dyn } = 2 \times 10 ^ { 11 } M _ { \odot } .