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Fig. 3


Radial gas temperature profiles in the mid-plane of the disk following the test of Pascucci et al. (2004) for τ = 0.1. We comparethe gas temperature computed using MCFOST (black dotted-line) and RADMC-3D (red dashed-line), the hybrid method (M1+FLD, blue dots) and the FLD method alone (orange dots) in RAMSES. Left: central star temperature T⋆,1 = 5800 K; right: T⋆,2 = 15 000 K.

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