Monte Carlo post-processing of radiation hydrodynamical protoplanetary disk models shows typical 10 percent temperature agreement, with systematic FLD/MCRT discrepancies that significantly alter predicted NIR and submm fluxes.
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Monte Carlo post-processing for radiation hydro simulations of accreting planets in protoplanetary disks
Monte Carlo post-processing of radiation hydrodynamical protoplanetary disk models shows typical 10 percent temperature agreement, with systematic FLD/MCRT discrepancies that significantly alter predicted NIR and submm fluxes.