Could merged star-clusters build up a small galaxy?

dc.creatorFellhauer, Michael
dc.creatorKroupa, Pavel
dc.date2000-01-14
dc.date2000-02-11
dc.date.accessioned2026-07-07T01:51:44Z
dc.date.available2026-07-07T01:51:44Z
dc.descriptionWe investigate the behaviour of a cluster of young massive star clusters (hereafter super-cluster) in the tidal field of a host galaxy with a high-resolution particle-mesh code, Superbox. Specifically we want to establish if and how such super star-clusters merge and carry out a detailed study of the resulting merger-object. This merger-object shows either the properties of a compact spherical object or the elongated (`fluffy') shape of dSph-galaxies depending on the initial concentration of the super-cluster.
dc.description6 pages, to appear in Massive Stellar Clusters, eds: A. Lancon, C. Boily, ASP Conf.Series, revised version has improved formatting
dc.identifierhttps://arxiv.org/abs/astro-ph/0001259
dc.identifierhttp://arxiv.org/abs/astro-ph/0001259
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/395
dc.subjectAstrophysics
dc.titleCould merged star-clusters build up a small galaxy?
dc.typetext

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