2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/7488We present results from a study of high- and low-ionization emission line ratios as a function of projected velocity for a sample of eight active galactic nuclei (AGNs). Our results are based on analysis of high signal-to-noise optical and Hubble Space Telescope (HST) UV spectra. Comparing the emission line ratios to those predicted by photoionization models indicates that the physical conditions responsible for the high-ionization emission lines are consistent with a wind, whereas those of the low-ionization lines are consistent with a virialized disk.5 pages, 2 figures in AASTeX. To appear in "AGN Physics with the Sloan Digital Sky Survey", ASP Conference Series Vol. 311, 2004, G. T. Richards and P. B. Hall, edsAstrophysicstext