Fig. 4.
Cross-section of the disk wind on the meridian plane including the angular-momentum axis of the precession and the direction of the jet ejection at a moment. The opening angle of the disk wind is assumed to be 2 × 60°. A bullet of the jet starts from the center, and first interacts with the disk-wind matter around the distance of vw Tp/2, which could cause the enhancement of the optical lines.