Structure and distribution of the density of our best-fit model for the disk and outflow of 89 Her. The lower inset shows a zoom into the innermost region of the outflow together with the rotating disk, with density values of ∼10⁶ and ≥10⁷ cm⁻³, respectively. The rest of the outflow presents density values ≤10⁵ cm⁻³. The expansion velocity is represented with arrows. The four horizontal blue dashed lines mark the former extent of the nebula in our previous model (see Gallardo Cava et al. 2021).