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Radiative transfer modelling in protoplanetary disks with the P‐N Approximation and Monte Carlo techniques
L. Graziani, L. Barletti, S. Aiello and C. Cecchi‐Pestellini Mathematical Methods in the Applied Sciences 33(10) 1263 (2010) https://doi.org/10.1002/mma.1285
Effects of scattering and dust grain size on the temperature structure of protoplanetary discs: a three-layer approach