Fig. 1
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Gas structure in the outer regions of the protoplanetary disk at different times, for our fiducial model with an initial disk size of R1 = 100 AU and an initial mass of 0.17 M⊙. Top: gas surface density profile from Eq. (1). Bottom: radial gas flux from Eq. (8). The dots illustrate the location where the gas moves outwards with time.
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