The tidal perturbation of the low-mass globular cluster NGC 5466

Simple item page
dc.creatorOdenkirchen, M.
dc.creatorGrebel, E. K.
dc.date2003-07-28
dc.date.accessioned2026-07-07T02:09:04Z
dc.date.available2026-07-07T02:09:04Z
dc.descriptionThe 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.
dc.description4 pages, to be published in the proceedings of the conference "Satellites and Tidal tails" held at La Palma, Canary Islands, May 26 -30, 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0307481
dc.identifierhttp://arxiv.org/abs/astro-ph/0307481
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6299
dc.subjectAstrophysics
dc.titleThe tidal perturbation of the low-mass globular cluster NGC 5466
dc.typetext

Files

Collections

arXiv