Simulated stellar wind of TOI-1860, DS Tuc A, and HD 63433 in the x_⋆ − y_⋆ plane. The rotation axis lies along the positive z_⋆. The Alfvén surface is shown as a translucent surface and its intersection on the x_⋆ − y_⋆ plane is shown as a white curve. The colour bar indicates the total wind velocity. The orbits of the hosted exoplanets are also included as coloured ellipses. For HD 63433, we also show the simulations from the 2023 data analysed in Bellotti et al. (2024).