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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/8489
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/8489 |
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3498 |
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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 Técnicas2025-09-29T10:15:21Zoai: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:34982025-09-29 10:15:22.118CONICET 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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1844614089563701248 |
score |
13.070432 |