Fig. 9.

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Distribution of the best-fitting model parameters for our sample galaxies. The parameters of the model are described in detail in Appendix E.1. For R.A., we only included galaxies with non-isotropic outflows (O.A. < 75°), and for P.A., we considered only galaxies with non-isotropic outflows (O.A. < 75°) that are also not seen nearly face on (R.A. < 75°). The median and standard deviation of each distribution are indicated in each corresponding panel. The best-fitting parameters and their uncertainties obtained for each galaxy are provided in Table D.2.
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