ρ = (dρ/dt)_inflow*t + ρ_0                                            for t << τ;
ρ = ρ_∞ = (dρ/dt)_inflow*τ                                           for t → ∞, where ρ_0 is the initial density at time zero whatever that is for the galaxy. We see that ρ saturates at ρ_∞ = (dρ/dt)_inflow*τ. Note, as the rate of outflow constant decreases (i.e., τ increases), the saturation density increases: i.e., τ ↑ ρ_∞ ↑.