Tidal tails around globular clusters

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dc.creatorMontuori, M.
dc.creatorCapuzzo-Dolcetta, R.
dc.creatorDi Matteo, P.
dc.creatorMiocchi, P.
dc.date2007-09-04
dc.date.accessioned2026-07-07T08:27:32Z
dc.date.available2026-07-07T08:27:32Z
dc.descriptionWe present the results of detailed N-body simulations of clusters moving in a realistic Milky Way (MW) potential. The strong interaction with the bulge and the disk of the Galaxy leads to the formation of tidal tails, emanating from opposite sides of the cluster. Their orientation and morphology may be interpreted easily in terms of a comoving frame of coordinates.
dc.description2 pages, 2 figures, presented at the Conference Pathways Through an Eclectic Universe, Tenerife, Spain, 3rd to 27th April, 2007, ASP Conf. Ser., in press
dc.identifierhttps://arxiv.org/abs/0709.0460
dc.identifierhttp://arxiv.org/abs/0709.0460
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/137302
dc.subjectAstrophysics
dc.titleTidal tails around globular clusters
dc.typetext

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