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dc.contributor.authorBalaha, Farah
dc.contributor.authorAlhosani, Maryam
dc.contributor.authorAsa'd, Randa
dc.contributor.authorChillingarian, Igor V.
dc.date.accessioned2020-02-19T09:07:16Z
dc.date.available2020-02-19T09:07:16Z
dc.date.issued2019
dc.identifier.citationFarah Balaha et al 2019 J. Phys.: Conf. Ser. 1258 012020en_US
dc.identifier.issn1742-6596
dc.identifier.urihttp://hdl.handle.net/11073/16614
dc.description.abstractIn this paper, we find the ages and metallicities of 8 Large Magellanic Cloud (LMC) star clusters obtained from integrated light spectra and use them to obtain the Chemical Enrichment History of the host galaxy. Our results are in good agreement with those obtained from resolved studies. This confirms that this method can be used for far away galaxies for which their star clusters are not resolved.en_US
dc.language.isoen_USen_US
dc.publisherIOP Scienceen_US
dc.relation.urihttps://doi.org/10.1088/1742-6596/1258/1/012020en_US
dc.titleUsing the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMCen_US
dc.typePeer-Revieweden_US
dc.typeArticleen_US
dc.typePublished versionen_US
dc.identifier.doi10.1088/1742-6596/1258/1/012020en_US


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