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We discuss the results of modelling of young magnetized stars, where matterflow is calculated using the three-dimensional (3D) magneto-hydrodynamic (MHD)"Cubed Sphere" code, and the spectra are calculated using the 3D Monte Carloradiative transfer code "TORUS". Two examples of modelling are shown: (1)accretion onto stars in stable and unstable regimes, and (2) accretion to ayoung star V2129 Oph, modelled with realistic parameters.

Simulations of Accretion onto Magnetized Stars: Results of 3D MHD Simulations and 3D Radiative Transfer