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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/ |