Left: radial gas temperature profile in the mid-plane of the disk following the test of Pinte et al. (2009). Right: vertical gas temperature profile at a cylindrical radius of 0.2 AU in the disk. We compare the gas temperature computed using RADMC-3D, the hybrid method (M1+FLD) and the FLD method alone in RAMSES. The integrated optical depth in the disk mid-plane is τ810 nm = 103 and the stellar temperature is T⋆ = 4000 K.
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