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Fig. 6
1000 AU disk edge-on slices of the radiative acceleration, following the test of Pascucci et al. (2004) obtained with RAMSES after stationarity is reached. Left: FLD run; right: hybrid run. Star and disk parameters: τ = 100 and T⋆,1. The hybrid radiative acceleration is about 100 times greater than the FLD one.
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