Spectroscopy of Globular Clusters in NGC 1399 - A Progress Report

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dc.creatorRichtler, T.
dc.creatorDirsch, B.
dc.creatorGeisler, D.
dc.creatorGebhardt, K.
dc.creatorHilker, M.
dc.creatorInfante, L.
dc.creatorMinniti, D.
dc.creatorRejkuba, M.
dc.creatorForte, J. C.
dc.creatorLarsen, S.
dc.creatorGrebel, E. K.
dc.creatorAlonso, V.
dc.date2001-08-08
dc.date.accessioned2026-07-07T01:59:36Z
dc.date.available2026-07-07T01:59:36Z
dc.descriptionWe performed spectroscopy of globular clusters associated with NGC 1399 and measured radial velocities of more than 400 clusters, the largest sample ever obtained for dynamical studies. In this progress report, we present the sample and the first preliminary results. Red and blue clusters have slightly different velocity dispersions in accordance with their different density profiles. Their velocity dispersions remain constant with radial distance, which differs from earlier work.
dc.description5 pages, 2 figures. To appear in the proceedings of IAU Symp. 207, "Extragalactic Star Clusters", eds. E.K. Grebel, D. Geisler and D. Minniti
dc.identifierhttps://arxiv.org/abs/astro-ph/0108140
dc.identifierhttp://arxiv.org/abs/astro-ph/0108140
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3177
dc.subjectAstrophysics
dc.titleSpectroscopy of Globular Clusters in NGC 1399 - A Progress Report
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