2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/8358We calculate multicomponent radiatively driven stellar wind models suitable for central stars of planetary nebulae. Some of these stellar winds may be adequately modelled using one-component models, however for some of them multicomponent models are necessary. We obtain a range of stellar parameters for different types of mass-loss.4 pages; to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. MoehlerAstrophysicstext