Profiles of the turbulent taylor number for each source. Top panel: turbulent taylor number Ta_t ≡ v_rot/σ_v of the extended rotating disks for the optical-emitting gas. Middle panel: turbulent taylor number for the compact rotating disks. Bottom panel: upper limits for the turbulent taylor number for the filamentary sources. The black dashed lines denote the transition between strong rain at T_at < 1 (turbulence dominated), mild rain (clumpy disk) at 1 < Ta_t < 3 (turbulence and rotation), and dominant disk Ta_t > 3 (rotation dominated).