2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/6299The distribution of stars in the outer part of the sparse globular cluster NGC 5466 provides evidence for possible tidal mass loss after a recent disk-shock near the solar circle.4 pages, to be published in the proceedings of the conference "Satellites and Tidal tails" held at La Palma, Canary Islands, May 26 -30, 2003AstrophysicsThe tidal perturbation of the low-mass globular cluster NGC 5466text