Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters

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We present metallicities for 15 Small Magellanic Cloud (SMC) star clusters. We add to this information the ages and metallicities of 15 additional star clusters previously studied by Parisi et al. (2009) and Parisi et al. (2013) which were observed and analyzed following the same procedures as in th...

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Detalles Bibliográficos
Autores principales:	Parisi, María Celeste, Clariá Olmedo, Juan José, Oddone, Mónica, Carraro, G., Geisler, D., Villanova, S., Costa, E., Grocholski, A. J., Sarajedini, A., Leiton, R.
Formato:	conferenceObject
Lenguaje:	Inglés
Publicado:	2021
Materias:	Star clusters Small magellanic cloud Metallicity
Acceso en línea:	http://hdl.handle.net/11086/18973
Aporte de:	Repositorio Digital Universitario (UNC) de Universidad Nacional de Córdoba

id	I10-R14111086-18973
record_format	dspace
institution	Universidad Nacional de Córdoba
institution_str	I-10
repository_str	R-141
collection	Repositorio Digital Universitario (UNC)
language	Inglés
topic	Star clusters Small magellanic cloud Metallicity
spellingShingle	Star clusters Small magellanic cloud Metallicity Parisi, María Celeste Clariá Olmedo, Juan José Oddone, Mónica Carraro, G. Geisler, D. Villanova, S. Costa, E. Grocholski, A. J. Sarajedini, A. Leiton, R. Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters
topic_facet	Star clusters Small magellanic cloud Metallicity
description	We present metallicities for 15 Small Magellanic Cloud (SMC) star clusters. We add to this information the ages and metallicities of 15 additional star clusters previously studied by Parisi et al. (2009) and Parisi et al. (2013) which were observed and analyzed following the same procedures as in the presentwork. Therefore, we compiled a sample of 30 SMC star clusters homogeneously studied. Metallicities are determined from the Calcium II triplet lines (CaT) in spectra obtained using FORS2 multiobject spectrograph on the VLT (Paranal, Chile) and ages are determined from Color-Magnitude Diagrams built from photometry on the pre-images. Using this sample, we now here analyze the chemical properties of the SMC, particularly the Age-Metallicity Relation. We found three new old clusters which help to fill the so called SMC "age gap" between L 1 and NGC121. These new old SMC clusters broadly increase our knowledge of the chemical evolution of this galaxy during the earliest epochs.
format	conferenceObject
author	Parisi, María Celeste Clariá Olmedo, Juan José Oddone, Mónica Carraro, G. Geisler, D. Villanova, S. Costa, E. Grocholski, A. J. Sarajedini, A. Leiton, R.
author_facet	Parisi, María Celeste Clariá Olmedo, Juan José Oddone, Mónica Carraro, G. Geisler, D. Villanova, S. Costa, E. Grocholski, A. J. Sarajedini, A. Leiton, R.
author_sort	Parisi, María Celeste
title	Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters
title_short	Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters
title_full	Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters
title_fullStr	Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters
title_full_unstemmed	Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters
title_sort	age and metallicity analysis of the small magellanic cloud from star clusters
publishDate	2021
url	http://hdl.handle.net/11086/18973
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bdutipo_str	Repositorios
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Age and Metallicity Analysis of the Small Magellanic Cloud from Star Clusters

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