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dc.date.accessioned 2019-10-30T13:47:07Z
dc.date.available 2019-10-30T13:47:07Z
dc.date.issued 2006
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84358
dc.description.abstract NGC 4649 (M60) is one of a handful of giant Virgo ellipticals. We have obtained Gemini/GMOS (Gemini North Multi-Object Spectrograph) spectra for 38 globular clusters (GCs) associated with this galaxy. Applying the multi-index χ2 minimization technique of Proctor and Sansom with the single stellar population models of Thomas, Maraston and Korn, we derive ages, metallicities and α-element abundance ratios. We find several young (2-3 Gyr old) supersolar metallicity GCs, while the majority are old (>10 Gyr), spanning a range of metallicities from solar to [Z/H] = -2. At least two of these young GCs are at large projected radii of 17-20 kpc. The galaxy itself shows no obvious signs of a recent starburst, interaction or merger. A trend of decreasing α-element ratio with increasing metallicity is found. en
dc.format.extent 325-334 es
dc.language en es
dc.subject Galaxies: individual: NGC 4649 es
dc.subject Galaxies: star clusters es
dc.subject Globular clusters: general es
dc.title Gemini/GMOS spectra of globular clusters in the Virgo giant elliptical NGC 4649 en
dc.type Articulo es
sedici.identifier.other doi:10.1111/j.1365-2966.2006.10097.x es
sedici.identifier.other eid:2-s2.0-33645806296 es
sedici.identifier.issn 0035-8711 es
sedici.creator.person Pierce, Michael es
sedici.creator.person Bridges, Terry es
sedici.creator.person Forbes, Duncan A. es
sedici.creator.person Proctor, Robert es
sedici.creator.person Beasley, Michael A. es
sedici.creator.person Gebhardt, Karl es
sedici.creator.person Faifer, Favio Raúl es
sedici.creator.person Forte, Juan Carlos es
sedici.creator.person Zepf, Stephen E. es
sedici.creator.person Sharpies, Ray es
sedici.creator.person Hanes, David A. es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Instituto de Astrofísica de La Plata 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 Monthly Notices of the Royal Astronomical Society es
sedici.relation.journalVolumeAndIssue vol. 368, no. 1 es
sedici.rights.sherpa * RoMEO: verde* Pre-print del autor: can* Post-print del autor: can* Versión de editor/PDF:can* Condiciones:>>El pre-print sólo puede depositarse antes de la aceptación>>Pre-print on author's personal website, employer website, free public server or pre-prints in subject area>>El pre-print debe acompañarse de una declaración establecida (ver enlace)>>Pre-print set statement must be amended upon publication (see policy)>>La versión de editor/PDF puede utilizarse>>Author's Post-print on Institutional repositories or Central repositories>>Publisher's version/PDF on Institutional repositories or Central repositories, with all rights reserved (see policy)>>La fuente editorial debe reconocerse>>Debe ir enlazado a la versión de editor>>La copia archivada debe acompañarse de la frase establecida (ver Política)* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/0035-8711/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)