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Major and minor axis kinematics of the stellar and gaseous component of a sample of 11 Low Surface Brightness galaxies is presented. The data, together with broad band imaging, will be used to construct detailed mass models aimed at deriving the central density radial prole of the dark matter component. The same data are used to study the Vcirc - sc relation for LSBs. We nd that LSBs have a higher Vcirc at a given sc(or lower sc at a given Vcirc) when compared to HSB and Ellipticals. This argues against the relevance of baryon collapse in the radial density prole of the dark matter haloes of LSB galaxies.

Low Surface Brighness galaxies: Vc-s0 relation and halo central density radial profile from stellar kinematics measurements