Azimuthally averaged local accretion rate, ṁ(r), at different times during the inward migration of the planet for the standard model (q = 0.001, ṁ = 10^-7, α = 0.003). The plot is similar to Fig. 4, which has the same parameters, but now for moving planets. To compare the accretion rate near the planet the position is rescaled to units of the disk scale height at the position of the planet. The labels refer to the elapsed time (in initial orbits) after the release of the planet.