Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy

Autores
Ahumada, Andrea Veronica; Vega, Luis Rodolfo; Clariá, Juan José; Oddone, Mónica Alejandra; Palma, Tali
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present flux-calibrated integrated spectra in the optical range (3700–6800 Å) obtained at Complejo Astronómico El Leoncito (CASLEO, Argentina) for a sample of 10 concentrated star clusters belonging to the Large Magellanic Cloud (LMC). No previous data exist for two of these objects (SL 142 and SL 624), while most of the remaining clusters have been only poorly studied. We derive simultaneously foreground E(B − V) reddening values and ages for the cluster sample by comparing their integrated spectra with template LMC cluster spectra and with two different sets of simple stellar population models. Cluster reddening values and ages are also derived from both available interstellar extinction maps and by using diagnostic diagrams involving the sum of equivalent widths of some selected spectral features and their calibrations with age, respectively. For the studied sample, we derive ages between 1 Myr and 240 Myr. In an effort to create a spectral library at the LMC metallicity level with several clusters per age range, the cluster sample presented here stands out as a useful complement to previous ones.
Fil: Ahumada, Andrea Veronica. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Vega, Luis Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Clariá, Juan José. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Oddone, Mónica Alejandra. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Palma, Tali. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Materia
GENERAL
MAGELLANIC CLOUDS – GALAXIES
SPECTROSCOPIC – (GALAXIES)
STAR CLUSTERS
TECHNIQUES
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/179871
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/179871
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopyAhumada, Andrea VeronicaVega, Luis RodolfoClariá, Juan JoséOddone, Mónica AlejandraPalma, TaliGENERALMAGELLANIC CLOUDS – GALAXIESSPECTROSCOPIC – (GALAXIES)STAR CLUSTERSTECHNIQUEShttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We present flux-calibrated integrated spectra in the optical range (3700–6800 Å) obtained at Complejo Astronómico El Leoncito (CASLEO, Argentina) for a sample of 10 concentrated star clusters belonging to the Large Magellanic Cloud (LMC). No previous data exist for two of these objects (SL 142 and SL 624), while most of the remaining clusters have been only poorly studied. We derive simultaneously foreground E(B − V) reddening values and ages for the cluster sample by comparing their integrated spectra with template LMC cluster spectra and with two different sets of simple stellar population models. Cluster reddening values and ages are also derived from both available interstellar extinction maps and by using diagnostic diagrams involving the sum of equivalent widths of some selected spectral features and their calibrations with age, respectively. For the studied sample, we derive ages between 1 Myr and 240 Myr. In an effort to create a spectral library at the LMC metallicity level with several clusters per age range, the cluster sample presented here stands out as a useful complement to previous ones.Fil: Ahumada, Andrea Veronica. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaFil: Vega, Luis Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Clariá, Juan José. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaFil: Oddone, Mónica Alejandra. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaFil: Palma, Tali. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaIOP Publishing2016-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/179871Ahumada, Andrea Veronica; Vega, Luis Rodolfo; Clariá, Juan José; Oddone, Mónica Alejandra; Palma, Tali; Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy; IOP Publishing; Publications of the Astronomical Society of the Pacific; 128; 967; 9-2016; 4101-41140004-6280CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1538-3873/128/967/094101info:eu-repo/semantics/altIdentifier/doi/10.1088/1538-3873/128/967/094101info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:43:36Zoai:ri.conicet.gov.ar:11336/179871instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:43:36.828CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
title Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
spellingShingle Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
Ahumada, Andrea Veronica
GENERAL
MAGELLANIC CLOUDS – GALAXIES
SPECTROSCOPIC – (GALAXIES)
STAR CLUSTERS
TECHNIQUES
title_short Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
title_full Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
title_fullStr Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
title_full_unstemmed Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
title_sort Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy
dc.creator.none.fl_str_mv Ahumada, Andrea Veronica
Vega, Luis Rodolfo
Clariá, Juan José
Oddone, Mónica Alejandra
Palma, Tali
author Ahumada, Andrea Veronica
author_facet Ahumada, Andrea Veronica
Vega, Luis Rodolfo
Clariá, Juan José
Oddone, Mónica Alejandra
Palma, Tali
author_role author
author2 Vega, Luis Rodolfo
Clariá, Juan José
Oddone, Mónica Alejandra
Palma, Tali
author2_role author
author
author
author
dc.subject.none.fl_str_mv GENERAL
MAGELLANIC CLOUDS – GALAXIES
SPECTROSCOPIC – (GALAXIES)
STAR CLUSTERS
TECHNIQUES
topic GENERAL
MAGELLANIC CLOUDS – GALAXIES
SPECTROSCOPIC – (GALAXIES)
STAR CLUSTERS
TECHNIQUES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present flux-calibrated integrated spectra in the optical range (3700–6800 Å) obtained at Complejo Astronómico El Leoncito (CASLEO, Argentina) for a sample of 10 concentrated star clusters belonging to the Large Magellanic Cloud (LMC). No previous data exist for two of these objects (SL 142 and SL 624), while most of the remaining clusters have been only poorly studied. We derive simultaneously foreground E(B − V) reddening values and ages for the cluster sample by comparing their integrated spectra with template LMC cluster spectra and with two different sets of simple stellar population models. Cluster reddening values and ages are also derived from both available interstellar extinction maps and by using diagnostic diagrams involving the sum of equivalent widths of some selected spectral features and their calibrations with age, respectively. For the studied sample, we derive ages between 1 Myr and 240 Myr. In an effort to create a spectral library at the LMC metallicity level with several clusters per age range, the cluster sample presented here stands out as a useful complement to previous ones.
Fil: Ahumada, Andrea Veronica. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Vega, Luis Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Clariá, Juan José. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Oddone, Mónica Alejandra. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Palma, Tali. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
description We present flux-calibrated integrated spectra in the optical range (3700–6800 Å) obtained at Complejo Astronómico El Leoncito (CASLEO, Argentina) for a sample of 10 concentrated star clusters belonging to the Large Magellanic Cloud (LMC). No previous data exist for two of these objects (SL 142 and SL 624), while most of the remaining clusters have been only poorly studied. We derive simultaneously foreground E(B − V) reddening values and ages for the cluster sample by comparing their integrated spectra with template LMC cluster spectra and with two different sets of simple stellar population models. Cluster reddening values and ages are also derived from both available interstellar extinction maps and by using diagnostic diagrams involving the sum of equivalent widths of some selected spectral features and their calibrations with age, respectively. For the studied sample, we derive ages between 1 Myr and 240 Myr. In an effort to create a spectral library at the LMC metallicity level with several clusters per age range, the cluster sample presented here stands out as a useful complement to previous ones.
publishDate 2016
dc.date.none.fl_str_mv 2016-09
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/179871
Ahumada, Andrea Veronica; Vega, Luis Rodolfo; Clariá, Juan José; Oddone, Mónica Alejandra; Palma, Tali; Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy; IOP Publishing; Publications of the Astronomical Society of the Pacific; 128; 967; 9-2016; 4101-4114
0004-6280
CONICET Digital
CONICET
url http://hdl.handle.net/11336/179871
identifier_str_mv Ahumada, Andrea Veronica; Vega, Luis Rodolfo; Clariá, Juan José; Oddone, Mónica Alejandra; Palma, Tali; Determination of reddening and age for ten large Magellanic Cloud star clusters from integrated spectroscopy; IOP Publishing; Publications of the Astronomical Society of the Pacific; 128; 967; 9-2016; 4101-4114
0004-6280
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1538-3873/128/967/094101
info:eu-repo/semantics/altIdentifier/doi/10.1088/1538-3873/128/967/094101
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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