Abstract
We have initiated a project that aims to revise the robustness of the suggestions of the dearth of dark matter in the central regions of barred galaxies through a detailed study of the galaxy NGC 3367. The internal kinematics of this galaxy has been measured in ionized and molecular gas and in the stellar component, making it a good benchmark for dynamical studies because it allows us to analyze the biases associated with each tracer. >From our observations we will directly measure the bar pattern speed, a property that has been considered as a free parameter in all previous studies.
