2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/6940Turbulent accretion disks are the most probable origin of jets from young stellar objects. Using an extended version of ZEUS-3D code in the axisymmetry option we investigate the evolution of a disk wind into a collimated jet. Resistive jets propagate slower with increasing magnetic diffusivity, and the degree of collimation decreases. The resistive disk included in the simulations ejects persistent, well collimated jet.To appear in: Stars as Suns: Activity, Evolution and Planets, eds. A. K. Dupree, A. Benz, IAU Symposium no. 219 ProceedingsAstrophysicstext