2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/9176We present the internal velocity dispersions and spectral line indices for six Virgo ultra-compact dwarf (UCD) galaxies obtained from spectroscopy with the Keck II 10-m telescope. We use these results: 1) to compare the Virgo UCDs with the Fornax UCD population; 2) to compare UCDs with globular clusters (GCs) to determine if UCDs and the most luminous GCs are the same or distinct systems; 3) to further test the nucleated dwarf elliptical (dE,N) stripping hypothesis for UCD formation.3 pages, 3 figures. To be published in the Proceedings IAUC198, 2005AstrophysicsThe Origin of UCDs in the Virgo Clustertext