2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/20232We complete the analysis of the equilibrium shapes of rotating self-gravitating gases initiated in Phys. Rev. Lett. 89 031101 (2002) (cond-mat/0202140) by studying the formation and thermodynamics of asymmetric binaries and by introducing a family of order parameters to classify the possible equilibrium states.4 pages, 5 figuresStatistical MechanicsAstrophysicstext