Gas accretion rates as a function of time of a forming giant planet, and accretion rate in the surrounding protoplanetary disk at the moment of transition into gas runaway accretion. The thick black solid line is the accretion rate of the planet Ṁ_XY. The thin solid black line is the disk-limited rate Ṁ_XY,max. The red dotted line is Ṁ_XY,max,F, the (non-equilibrium) flow-limited maximal accretion rate, while the rate limited by the local reservoir is shown by the magenta dashed-dotted line (Ṁ_XY,max,R). The cyan long-dashed-dotted line shows M_feed/dt. The accretion rate in the disk inside the planet’s position, Ṁ_I, is the blue dashed line, while the accretion rate in the disk outside the planet’s position Ṁ_O is the green long-dashed line.