A method to deconvolve stellar rotational velocities - III. The probability distribution function via maximum likelihood utilizing finite distribution mixturesR. Orellana, P. Escárate, M. Curé, A. Christen, R. Carvajal and J. C. AgüeroA&A, 623 (2019) A138DOI: https://doi.org/10.1051/0004-6361/201833455
