Two newly identified, relatively old star clusters in the Small Magellanic Cloud
- Autores
- Piatti, Andres Eduardo; Sarajedini, Ata; Geisler, Doug; Gallart, Carme; Wischnjewsky, Marina
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the results on the age and metallicity estimates of the Small Magellanic Cloud (SMC) clusters L110, L112 and L113 obtained from CCD Washington CT1 photometry. We confirm L113 as a relatively old and metal-poor cluster, and report for the first time that L110 and 112 are also relatively old clusters (t ~ 6.5 Gyr). Their derived ages and metallicities reinforce previous suggestions that the farther a cluster is from the centre of the galaxy, the older and more metal-poor it is, with some dispersion. In addition, the bursting star formation model still appears to be the most probable paradigm to describe the SMC´s star formation history. We call attention to a second possible burst at ~6-7 Gyr, besides the known burst at ~3 Gyr.
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Sarajedini, Ata. University of Florida; Estados Unidos
Fil: Geisler, Doug. Universidad de Concepción; Chile
Fil: Gallart, Carme. Instituto de Astrof´ısica de Canarias; España
Fil: Wischnjewsky, Marina. - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/21048
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Two newly identified, relatively old star clusters in the Small Magellanic CloudPiatti, Andres EduardoSarajedini, AtaGeisler, DougGallart, CarmeWischnjewsky, Marinahttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the results on the age and metallicity estimates of the Small Magellanic Cloud (SMC) clusters L110, L112 and L113 obtained from CCD Washington CT<sub>1</sub> photometry. We confirm L113 as a relatively old and metal-poor cluster, and report for the first time that L110 and 112 are also relatively old clusters (t ~ 6.5 Gyr). Their derived ages and metallicities reinforce previous suggestions that the farther a cluster is from the centre of the galaxy, the older and more metal-poor it is, with some dispersion. In addition, the bursting star formation model still appears to be the most probable paradigm to describe the SMC´s star formation history. We call attention to a second possible burst at ~6-7 Gyr, besides the known burst at ~3 Gyr.Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Sarajedini, Ata. University of Florida; Estados UnidosFil: Geisler, Doug. Universidad de Concepción; ChileFil: Gallart, Carme. Instituto de Astrof´ısica de Canarias; EspañaFil: Wischnjewsky, Marina.Oxford University Press2007-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21048Piatti, Andres Eduardo; Sarajedini, Ata; Geisler, Doug; Gallart, Carme; Wischnjewsky, Marina; Two newly identified, relatively old star clusters in the Small Magellanic Cloud; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 381; 1; 12-2007; L84-L880035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2007.00373.xinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnrasl/article-lookup/doi/10.1111/j.1745-3933.2007.00373.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:28:47Zoai:ri.conicet.gov.ar:11336/21048instacron: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 10:28:48.254CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
title |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
spellingShingle |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud Piatti, Andres Eduardo |
title_short |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
title_full |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
title_fullStr |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
title_full_unstemmed |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
title_sort |
Two newly identified, relatively old star clusters in the Small Magellanic Cloud |
dc.creator.none.fl_str_mv |
Piatti, Andres Eduardo Sarajedini, Ata Geisler, Doug Gallart, Carme Wischnjewsky, Marina |
author |
Piatti, Andres Eduardo |
author_facet |
Piatti, Andres Eduardo Sarajedini, Ata Geisler, Doug Gallart, Carme Wischnjewsky, Marina |
author_role |
author |
author2 |
Sarajedini, Ata Geisler, Doug Gallart, Carme Wischnjewsky, Marina |
author2_role |
author author author author |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present the results on the age and metallicity estimates of the Small Magellanic Cloud (SMC) clusters L110, L112 and L113 obtained from CCD Washington CT<sub>1</sub> photometry. We confirm L113 as a relatively old and metal-poor cluster, and report for the first time that L110 and 112 are also relatively old clusters (t ~ 6.5 Gyr). Their derived ages and metallicities reinforce previous suggestions that the farther a cluster is from the centre of the galaxy, the older and more metal-poor it is, with some dispersion. In addition, the bursting star formation model still appears to be the most probable paradigm to describe the SMC´s star formation history. We call attention to a second possible burst at ~6-7 Gyr, besides the known burst at ~3 Gyr. Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Sarajedini, Ata. University of Florida; Estados Unidos Fil: Geisler, Doug. Universidad de Concepción; Chile Fil: Gallart, Carme. Instituto de Astrof´ısica de Canarias; España Fil: Wischnjewsky, Marina. |
description |
We present the results on the age and metallicity estimates of the Small Magellanic Cloud (SMC) clusters L110, L112 and L113 obtained from CCD Washington CT<sub>1</sub> photometry. We confirm L113 as a relatively old and metal-poor cluster, and report for the first time that L110 and 112 are also relatively old clusters (t ~ 6.5 Gyr). Their derived ages and metallicities reinforce previous suggestions that the farther a cluster is from the centre of the galaxy, the older and more metal-poor it is, with some dispersion. In addition, the bursting star formation model still appears to be the most probable paradigm to describe the SMC´s star formation history. We call attention to a second possible burst at ~6-7 Gyr, besides the known burst at ~3 Gyr. |
publishDate |
2007 |
dc.date.none.fl_str_mv |
2007-12 |
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/11336/21048 Piatti, Andres Eduardo; Sarajedini, Ata; Geisler, Doug; Gallart, Carme; Wischnjewsky, Marina; Two newly identified, relatively old star clusters in the Small Magellanic Cloud; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 381; 1; 12-2007; L84-L88 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/21048 |
identifier_str_mv |
Piatti, Andres Eduardo; Sarajedini, Ata; Geisler, Doug; Gallart, Carme; Wischnjewsky, Marina; Two newly identified, relatively old star clusters in the Small Magellanic Cloud; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 381; 1; 12-2007; L84-L88 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2007.00373.x info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnrasl/article-lookup/doi/10.1111/j.1745-3933.2007.00373.x |
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 |
dc.publisher.none.fl_str_mv |
Oxford University Press |
publisher.none.fl_str_mv |
Oxford University Press |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |