Title Spatial distribution of stellar rotational axes of Be stars abstract: In order to know the distribution of rotational velocities of Be stars, a standard assumption is used, namely that the rotational axes are uniformed distributed. We use here polarimetric projected angles data from ca. 500 Be stars and make a statistical analysis. Furthermore we perform a Monte-Carlo simulation that explain the observed features of the angles, confirming that it is indeed uniform distributed, but the projected angles possess a bimodal structure. This last features may change the conclusion about the velocity distribution of these stars.