1 Introduction

We have recently begun to publish results on the kinematics of the stars in the inner region of spiral galaxies (Héraudeau & Simien 1998, hereafter Paper I). Our initial aim was to obtain central kinematical data on a significant sample of bright, nearby spirals with, as much as possible, available surface photometry. Here, we present the reduction of a second, more recent set of data. We have followed closely the method of Paper I at every step of the work, and only limited explanations are given in the present paper.