ASPCS
 
Back to Volume
Paper: Simulations of Accretion onto Magnetized Stars: Results of 3D MHD Simulations and 3D Radiative Transfer
Volume: 488, 8th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM 2013)
Page: 127
Authors: Romanova, M.; Kurosawa, R.
Abstract: We discuss the results of modelling of young magnetized stars, where matter flow is calculated using the three-dimensional (3D) magneto-hydrodynamic (MHD) Cubed Sphere code, and the spectra are calculated using the 3D Monte Carlo radiative transfer code TORUS. Two examples of modelling are shown: (1) accretion onto stars in stable and unstable regimes, and (2) accretion to a young star V2129 Oph, modelled with realistic parameters.
Back to Volume