Brγ emission region image of the magnetospheric accretion region of an RU Lup-like system at the Brγ peak wavelength, obtained from radiative transfer modelling with MCFOST. Depicted here are the accretion columns at the line centre, the star and the shock region at high latitude, as well as a contribution coming from a faint magnetospheric continuum. The model is axisymmetric, i.e. the magnetic axis is aligned with the stellar rotational axis, i.e. the vertical axis in the image above.