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dc.date.accessioned 2019-05-27T17:34:37Z
dc.date.available 2019-05-27T17:34:37Z
dc.date.issued 2017-08-15
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/75480
dc.description.abstract The giant elliptical galaxy NGC1316 is the brightest galaxy in the Fornax cluster, and displays a number of morphological features that might be interpreted as an intermediate age merger remanent ( 3 Gyr). Based on the idea that globular clusters systems (GCS) constitute genuine tracers of the formation and evolution of their host galaxies, we conducted a spectroscopic study of approximately 40 globular clusters (GCs) candidates associated with this interesting galaxy. We determined ages, metallicities, and a-element abundances for each GC present in the sample, through the measurement of different Lick indices and their subsequent comparison with simple stellar populations models (SSPs). es
dc.language en es
dc.subject astrofísica es
dc.subject elliptical galaxies; globular clusters; galaxy haloes en
dc.subject galaxias es
dc.title Deep MOS Spectroscopy of NGC1316 Globular Clusters en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.3390/galaxies5030039
sedici.creator.person Sesto, Leandro Alberto es
sedici.creator.person Faifer, Favio Raúl es
sedici.creator.person Forte, Juan Carlos es
sedici.creator.person Smith Castelli, Analía Viviana es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Comunicacion 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 Galaxies es
sedici.relation.journalVolumeAndIssue vol. 5, no. 3 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)