Simulation results in the IH domain for HD 147513 driven by the SH-ZDI magnetic field maps. The central white sphere denotes the boundary with the SC domain at 25 R_∗ (Sect. 3.1). The density structure of the steady-state solution is displayed on the equatorial plane (left) and the astrospheric current sheet (right). In the left panel, the topology and associated magnitudes of the dominant radial velocity components (u_r) of the stellar wind are also included (fast: green – slow: magenta). Selected 3D magnetic field lines are shown in white.