2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/6050Radial velocities were measured for 5 potential post-AGB stars, two in the globular cluster NGC 1851 and three in the dSph galaxy Ursa Minor. All five potential PAGB stars were found to be radial velocity non-members.Astrophysicstext