The conical wind/jet from a slowly rotating star at time
. The background shows the poloidal matter flux density and the lines show the poloidal projections of the magnetic field. The red vectors show the poloidal matter velocity . Dimensional values can be obtained from Table 1. For example for a CTTS, , , corresponds to 315 days, and the simulation region is 0.39 AU in radius. The horizontal axis shows the distance from the star in units of the reference radius . For this case and .