dc.date.accessioned2020-03-11T20:34:55Z
dc.date.accessioned2022-10-18T22:59:21Z
dc.date.available2020-03-11T20:34:55Z
dc.date.available2022-10-18T22:59:21Z
dc.date.created2020-03-11T20:34:55Z
dc.date.issued2010
dc.identifierhttp://hdl.handle.net/10533/240426
dc.identifier15010003
dc.identifierWOS:000273021000031
dc.identifierno scielo
dc.identifiereid=2-s2.0-77950248768
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4471765
dc.description.abstractWe present new integrated light spectroscopy of globular clusters (GCs) in NGC 5128, a nearby giant elliptical galaxy less than 4 Mpc away, in order to measure radial velocities and derive ages, metallicities, and alpha-element abundance ratios. Using the
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/708/2/1335
dc.relation10.1088/0004-637X/708/2/1335
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe Ages, Metallicities, and Alpha Element Enhancements of Globular Clusters in the Elliptical NGC 5128: A Homogeneous Spectroscopic Study with Gemini/Gemini Multi-Object Spectrograph
dc.typeArticulo


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