Surface density around a 60-Jupiter-mass planet in a viscous (α = 2   ×   10^-2) disk after 10⁴ orbits, with and without accretion onto the planet (dotted and solid gray line, respectively). The solid black line is the analytical fit using Eq. (1) with parameters that also fit the MIDI data (w = 0.36). The dashed line denotes r_exp, the radius where the surface density starts to deviate from a power law.