Critical study of the distribution of rotational velocities of Be stars - I. Deconvolution methods, effects due to gravity darkening, macroturbulence, and binarity
J. Zorec, Y. Frémat, A. Domiciano de Souza, F. Royer, L. Cidale, A.-M. Hubert, T. Semaan, C. Martayan, Y. R. Cochetti, M. L. Arias, Y. Aidelman and P. Stee