Notes. Columns for the torus or disk components are as follows. d is the ALMA MSR 870 μm torus size (diameter of the extended component at the 3σ level) and PA_A the position angle PA and inclination, from GB21. ^( * )The 870 μm PA is not along the equatorial direction (i.e., torus). The torus or disk inclination (i_torus) constraints from modeling of the IR emission with the CLUMPY torus models are from Alonso-Herrero et al. (2011, 2012), Ruschel-Dutra et al. (2014), Ichikawa et al. (2015), García-Bernete et al. (2019), Martínez-Paredes et al. (2020), the CAT3D-WIND models from González-Martín et al. (2019), and from modeling of X-ray observations are from Walton et al. (2010), Tanimoto et al. (2020), Ogawa et al. (2021). The torus inclinations from the ALMA MSR 870 μm images are from GB21 and from the ALMA CO(3−2) and CO(2−1) kinematics are from Alonso-Herrero et al. (2018, 2019) and GB21. Columns for the wind components are as follows. The ionization cone inclination (i_cone) constraints are from the modeling of the NLR by Fischer et al. (2013). PA_cone is the position angle of the ionization cones and the references are given in the text in Sect. 3.4. The wind-to-disk ratio f_wd constraints are from modeling with the CAT3D-WIND models from González-Martín et al. (2019).