On a possible origin for the lack of old star clusters in the Small Magellanic Cloud

Autores
Carpintero, Daniel Diego; Gómez, F. A.; Piatti, Andres Eduardo
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We model the dynamical interaction between the Small and LargeMagellanic Clouds and their corresponding stellar cluster populations. Our goal is to explore whether the lack of old clusters (>7 Gyr) in the Small Magellanic Cloud (SMC) can be the result of the capture of clusters by the Large Magellanic Cloud (LMC) as well as their ejection due to the tidal interaction between the two galaxies. For this purpose, we perform a suite of numerical simulations probing a wide range of parameters for the orbit of the SMC about the LMC. We find that, for orbital eccentricities e ≥ 0.4, approximately 15 per cent of the SMC clusters are captured by the LMC. In addition, another 20?50 per cent of its clusters are ejected into the intergalactic medium. In general, the clusters lost by the SMC are the less tightly bound cluster population. The final LMC cluster distribution shows a spatial segregation between clusters that originally belonged to the LMC and those that were captured from the SMC. Clusters that originally belonged to the SMC are more likely to be found in the outskirts of the LMC. Within this scenario, it is possible to interpret the difference observed between the star field and cluster SMC age?metallicity relationships for ages 7 Gyr.
Fil: Carpintero, Daniel Diego. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Gómez, F. A.. Michigan State University; Estados Unidos
Fil: Piatti, Andres Eduardo. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
Materia
Numerical methods
Small Magellanic Cloud
Magellanic Clouds
Star clusters
Galaxies
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:11336/8489
Acceder
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network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling On a possible origin for the lack of old star clusters in the Small Magellanic CloudCarpintero, Daniel DiegoGómez, F. A.Piatti, Andres EduardoNumerical methodsSmall Magellanic CloudMagellanic CloudsStar clustersGalaxieshttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We model the dynamical interaction between the Small and LargeMagellanic Clouds and their corresponding stellar cluster populations. Our goal is to explore whether the lack of old clusters (>7 Gyr) in the Small Magellanic Cloud (SMC) can be the result of the capture of clusters by the Large Magellanic Cloud (LMC) as well as their ejection due to the tidal interaction between the two galaxies. For this purpose, we perform a suite of numerical simulations probing a wide range of parameters for the orbit of the SMC about the LMC. We find that, for orbital eccentricities e ≥ 0.4, approximately 15 per cent of the SMC clusters are captured by the LMC. In addition, another 20?50 per cent of its clusters are ejected into the intergalactic medium. In general, the clusters lost by the SMC are the less tightly bound cluster population. The final LMC cluster distribution shows a spatial segregation between clusters that originally belonged to the LMC and those that were captured from the SMC. Clusters that originally belonged to the SMC are more likely to be found in the outskirts of the LMC. Within this scenario, it is possible to interpret the difference observed between the star field and cluster SMC age?metallicity relationships for ages 7 Gyr.Fil: Carpintero, Daniel Diego. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Gómez, F. A.. Michigan State University; Estados UnidosFil: Piatti, Andres Eduardo. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; ArgentinaWiley2013-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/8489Carpintero, Daniel Diego; Gómez, F. A.; Piatti, Andres Eduardo; On a possible origin for the lack of old star clusters in the Small Magellanic Cloud; Wiley; Monthly Notices Of The Royal Astronomical Society; 435; 1; 10-2013; 63-670035-8711enginfo:eu-repo/semantics/altIdentifier/url/http://mnrasl.oxfordjournals.org/content/435/1/L63info:eu-repo/semantics/altIdentifier/url/http://dx.doi.org/doi:10.1093/mnrasl/slt096info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1307.6231v1info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:45:35Zoai:ri.conicet.gov.ar:11336/8489instacron: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:34982025-10-22 11:45:35.346CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
title On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
spellingShingle On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
Carpintero, Daniel Diego
Numerical methods
Small Magellanic Cloud
Magellanic Clouds
Star clusters
Galaxies
title_short On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
title_full On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
title_fullStr On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
title_full_unstemmed On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
title_sort On a possible origin for the lack of old star clusters in the Small Magellanic Cloud
dc.creator.none.fl_str_mv Carpintero, Daniel Diego
Gómez, F. A.
Piatti, Andres Eduardo
author Carpintero, Daniel Diego
author_facet Carpintero, Daniel Diego
Gómez, F. A.
Piatti, Andres Eduardo
author_role author
author2 Gómez, F. A.
Piatti, Andres Eduardo
author2_role author
author
dc.subject.none.fl_str_mv Numerical methods
Small Magellanic Cloud
Magellanic Clouds
Star clusters
Galaxies
topic Numerical methods
Small Magellanic Cloud
Magellanic Clouds
Star clusters
Galaxies
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We model the dynamical interaction between the Small and LargeMagellanic Clouds and their corresponding stellar cluster populations. Our goal is to explore whether the lack of old clusters (>7 Gyr) in the Small Magellanic Cloud (SMC) can be the result of the capture of clusters by the Large Magellanic Cloud (LMC) as well as their ejection due to the tidal interaction between the two galaxies. For this purpose, we perform a suite of numerical simulations probing a wide range of parameters for the orbit of the SMC about the LMC. We find that, for orbital eccentricities e ≥ 0.4, approximately 15 per cent of the SMC clusters are captured by the LMC. In addition, another 20?50 per cent of its clusters are ejected into the intergalactic medium. In general, the clusters lost by the SMC are the less tightly bound cluster population. The final LMC cluster distribution shows a spatial segregation between clusters that originally belonged to the LMC and those that were captured from the SMC. Clusters that originally belonged to the SMC are more likely to be found in the outskirts of the LMC. Within this scenario, it is possible to interpret the difference observed between the star field and cluster SMC age?metallicity relationships for ages 7 Gyr.
Fil: Carpintero, Daniel Diego. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Gómez, F. A.. Michigan State University; Estados Unidos
Fil: Piatti, Andres Eduardo. Universidad Nacional de Cordoba. Observatorio Astronomico de Cordoba; Argentina
description We model the dynamical interaction between the Small and LargeMagellanic Clouds and their corresponding stellar cluster populations. Our goal is to explore whether the lack of old clusters (>7 Gyr) in the Small Magellanic Cloud (SMC) can be the result of the capture of clusters by the Large Magellanic Cloud (LMC) as well as their ejection due to the tidal interaction between the two galaxies. For this purpose, we perform a suite of numerical simulations probing a wide range of parameters for the orbit of the SMC about the LMC. We find that, for orbital eccentricities e ≥ 0.4, approximately 15 per cent of the SMC clusters are captured by the LMC. In addition, another 20?50 per cent of its clusters are ejected into the intergalactic medium. In general, the clusters lost by the SMC are the less tightly bound cluster population. The final LMC cluster distribution shows a spatial segregation between clusters that originally belonged to the LMC and those that were captured from the SMC. Clusters that originally belonged to the SMC are more likely to be found in the outskirts of the LMC. Within this scenario, it is possible to interpret the difference observed between the star field and cluster SMC age?metallicity relationships for ages 7 Gyr.
publishDate 2013
dc.date.none.fl_str_mv 2013-10
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/11336/8489
Carpintero, Daniel Diego; Gómez, F. A.; Piatti, Andres Eduardo; On a possible origin for the lack of old star clusters in the Small Magellanic Cloud; Wiley; Monthly Notices Of The Royal Astronomical Society; 435; 1; 10-2013; 63-67
0035-8711
url http://hdl.handle.net/11336/8489
identifier_str_mv Carpintero, Daniel Diego; Gómez, F. A.; Piatti, Andres Eduardo; On a possible origin for the lack of old star clusters in the Small Magellanic Cloud; Wiley; Monthly Notices Of The Royal Astronomical Society; 435; 1; 10-2013; 63-67
0035-8711
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://mnrasl.oxfordjournals.org/content/435/1/L63
info:eu-repo/semantics/altIdentifier/url/http://dx.doi.org/doi:10.1093/mnrasl/slt096
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1307.6231v1
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
dc.publisher.none.fl_str_mv Wiley
publisher.none.fl_str_mv Wiley
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 12.982451

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