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dc.date.accessioned 2019-10-30T18:15:43Z
dc.date.available 2019-10-30T18:15:43Z
dc.date.issued 2004
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84446
dc.description.abstract Radial velocities of 468 globular clusters around NGC 1399, the central galaxy in the Fornax cluster, have been obtained with FORS2 and the Mask Exchange Unit (MXU) at the ESO Very Large Telescope. This is the largest sample of globular cluster velocities around any galaxy obtained so far. The mean velocity uncertainty is 50 km s-1. This data sample is accurate and large enough to be used in studies of the mass distribution of NGC 1399 and the properties of its globular cluster system. Here we describe the observations and the reduction procedure, and we discuss the uncertainties of the resulting velocities. The complete sample of cluster velocities that is used in a dynamical study of NGC 1399 is tabulated. A subsample is compared with previously published values. en
dc.format.extent 2114-2132 es
dc.language en es
dc.subject Dark matter es
dc.subject Galaxies: elliptical and lenticular, cD es
dc.subject Galaxies: halos es
dc.subject Galaxies: individual (NGC 1399) es
dc.subject Galaxies: kinematics and dynamics es
dc.subject Galaxies: star clusters es
dc.title The globular cluster system of NGC 1399. III. VLT spectroscopy and database en
dc.type Articulo es
sedici.identifier.other doi:10.1086/380607 es
sedici.identifier.other eid:2-s2.0-17544403422 es
sedici.identifier.issn 0004-6256 es
sedici.creator.person Dirsch, B. es
sedici.creator.person Richtler, Thomas es
sedici.creator.person Geisler, D. es
sedici.creator.person Gebhardt, K. es
sedici.creator.person Hilker, M. es
sedici.creator.person Alonso, M. V. es
sedici.creator.person Forte, Juan Carlos es
sedici.creator.person Grebel, E. K. es
sedici.creator.person Infante, L. es
sedici.creator.person Larsen, S. es
sedici.creator.person Minniti, D. es
sedici.creator.person Rejkuba, M. es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle The Astronomical Journal es
sedici.relation.journalVolumeAndIssue vol. 127, no. 4 es
sedici.rights.sherpa * RoMEO: verde* Pre-print del autor: can* Post-print del autor: can* Versión de editor/PDF:can* Condiciones:>>On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository.>>Publisher's version/PDF may be used on any website or authors' institutional repository>>Deben reconocerse el copyright y la fuente editorial>>Debe ir enlazado a la versión de editor>>La versión de editor/PDF puede utilizarse>>Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article � a "non-exclusive licence to distribute">>Publisher last contacted on 10/02/2016>>Publisher last reviewed on 15/08/2017* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/0004-6256/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)