Modeling results for the magnetospheric accretion models (Thanathibodee et al. 2019a). Left: results for the wing subcomponent. Right: results for the core subcomponent. First row: Hα. Second row: Hβ. Each left subpanel corresponds to the fit performed on the [−50; +50] km/s range, while the right subpanels correspond to the fit on the full the line width ([−250; +250] km/s). The red line is the best model, while the colored lines represent a sample of the lowest ${\chi }_r^2$ models. The models are able to reproduce the deep absorption features of the wing component and reproduce the general shape of the core component.