A study of the recent chemical evolution of the Large Magellanic Cloud

Abstract: we present the results of a study of the Large Magellanic Cloud (LMC) chemical evolution during the last 2.2 Gyr. This study is based on Washington photometric observations of LMC's star clusters carried out with the Cerro Tololo Inter-American Observatory (CTIO) 4 m telescope, using...

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Main Authors: Palma, Tali., Clariá Olmedo, Juan José., Geisler, D., Ahumada, Andrea.
Format: conferenceObject
Language:eng
Published: 2021
Subjects:
Online Access:http://hdl.handle.net/11086/18969
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author Palma, Tali.
Clariá Olmedo, Juan José.
Geisler, D.
Ahumada, Andrea.
author_facet Palma, Tali.
Clariá Olmedo, Juan José.
Geisler, D.
Ahumada, Andrea.
author_sort Palma, Tali.
collection Repositorio Digital Universitario
description Abstract: we present the results of a study of the Large Magellanic Cloud (LMC) chemical evolution during the last 2.2 Gyr. This study is based on Washington photometric observations of LMC's star clusters carried out with the Cerro Tololo Inter-American Observatory (CTIO) 4 m telescope, using the C and T_1 filters. As tracers of the LMC's chemical enrichment we used 83 star clusters, from which 40 clusters are projected onto the bar region, 23 in the inner disc and 20 in the outer disc. More than half of the total sample has not been previously studied. We determine size, reddening, deprojected distance, age and metallicity of the observed star clusters.
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spelling rdu-unc.189692024-05-31T16:59:19Z A study of the recent chemical evolution of the Large Magellanic Cloud Palma, Tali. Clariá Olmedo, Juan José. Geisler, D. Ahumada, Andrea. Large Magellanic Cloud. Star Cluster. Washington photometry. Abstract: we present the results of a study of the Large Magellanic Cloud (LMC) chemical evolution during the last 2.2 Gyr. This study is based on Washington photometric observations of LMC's star clusters carried out with the Cerro Tololo Inter-American Observatory (CTIO) 4 m telescope, using the C and T_1 filters. As tracers of the LMC's chemical enrichment we used 83 star clusters, from which 40 clusters are projected onto the bar region, 23 in the inner disc and 20 in the outer disc. More than half of the total sample has not been previously studied. We determine size, reddening, deprojected distance, age and metallicity of the observed star clusters. Fil: Palma, Tali. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Palma, Tali. Ministerio de Ciencia, Tecnología e Innovación de la Nación. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Fil: Clariá Olmedo, Juan José. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Clariá Olmedo, Juan José. Ministerio de Ciencia, Tecnología e Innovación de la Nación. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Fil: Ahumada, Andrea. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Ahumada, Andrea. Ministerio de Ciencia, Tecnología e Innovación de la Nación. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Fil: Palma, Tali. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Palma, Tali. Ministerio de Ciencia, Tecnología e Innovación de la Nación. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Fil: Clariá Olmedo, Juan José. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Clariá Olmedo, Juan José. Ministerio de Ciencia, Tecnología e Innovación de la Nación. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Fil: Ahumada, Andrea. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Ahumada, Andrea. Ministerio de Ciencia, Tecnología e Innovación de la Nación. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Astronomía (incluye Astrofísica y Ciencias del Espacio) 2021-07-10T16:14:12Z 2021-07-10T16:14:12Z 2014 conferenceObject http://hdl.handle.net/11086/18969 eng Attribution-NonCommercial-ShareAlike 4.0 International https://creativecommons.org/licenses/by-nc-sa/4.0/ Impreso
spellingShingle Large Magellanic Cloud.
Star Cluster.
Washington photometry.
Palma, Tali.
Clariá Olmedo, Juan José.
Geisler, D.
Ahumada, Andrea.
A study of the recent chemical evolution of the Large Magellanic Cloud
title A study of the recent chemical evolution of the Large Magellanic Cloud
title_full A study of the recent chemical evolution of the Large Magellanic Cloud
title_fullStr A study of the recent chemical evolution of the Large Magellanic Cloud
title_full_unstemmed A study of the recent chemical evolution of the Large Magellanic Cloud
title_short A study of the recent chemical evolution of the Large Magellanic Cloud
title_sort study of the recent chemical evolution of the large magellanic cloud
topic Large Magellanic Cloud.
Star Cluster.
Washington photometry.
url http://hdl.handle.net/11086/18969
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