2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/5775We review the evidence for young stellar populations in the inner (< 200 pc) regions of Active Galactic Nuclei (AGN), and the physical mechanisms through which the stars can potentially create the emission lines that characterize AGN.Invited talk in 'Winds, Bubbles and Explosions' (Patzcuaro, Mexico, Sep. 2002), 6 pages, 3 figuresAstrophysicstext