A hidden link in the LMC star cluster formation history

Autores
Piatti, Andres Eduardo
Año de publicación
2025
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The age distribution function of star clusters in the Large Magellanic Cloud (LMC) is known to present a feature called the cluster age gap, a period of time from ∼ 4 to 11 Gyr ago with a remarkable small number of clusters identified. In this work we performed an in-depth analysis of three recently catalogued age gap cluster candidates with the aim of confirming their physical nature. We used GEMINI@GMOS g, i pho- tometry centred on the objects to build colour-magnitude diagrams from which we recognised their main features. We also performed an automatic search of stellar over- densities using Gaussian mixture model techniques and analysed the corresponding colour-magnitude diagrams similarly as performed for the aforementioned candidates. The present GEMINI data sets would seem to discard any strong evidence of these object being real clusters, and rather support the possibility of the result of stellar density variations of the LMC field star distribution. These three objects, in addition to other 17 new identified candidates, are placed in the LMC outermost disc in a limited region toward the southwest from the LMC centre. They had embraced the possibility to answer the long-time conundrum about the absence of LMC age gap clusters. From an statistical approach, combined with the knowledge of the expected LMC age-metallicity relationship, and recent simulations of the interaction between the LMC and the Milky Way, we provide not only evidence against the physical nature of the studied objects, but also an interpretation on the lack of identification of more LMC age gap clusters.
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Materia
cluster
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:11336/278764

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spelling A hidden link in the LMC star cluster formation historyPiatti, Andres Eduardoclusterhttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1The age distribution function of star clusters in the Large Magellanic Cloud (LMC) is known to present a feature called the cluster age gap, a period of time from ∼ 4 to 11 Gyr ago with a remarkable small number of clusters identified. In this work we performed an in-depth analysis of three recently catalogued age gap cluster candidates with the aim of confirming their physical nature. We used GEMINI@GMOS g, i pho- tometry centred on the objects to build colour-magnitude diagrams from which we recognised their main features. We also performed an automatic search of stellar over- densities using Gaussian mixture model techniques and analysed the corresponding colour-magnitude diagrams similarly as performed for the aforementioned candidates. The present GEMINI data sets would seem to discard any strong evidence of these object being real clusters, and rather support the possibility of the result of stellar density variations of the LMC field star distribution. These three objects, in addition to other 17 new identified candidates, are placed in the LMC outermost disc in a limited region toward the southwest from the LMC centre. They had embraced the possibility to answer the long-time conundrum about the absence of LMC age gap clusters. From an statistical approach, combined with the knowledge of the expected LMC age-metallicity relationship, and recent simulations of the interaction between the LMC and the Milky Way, we provide not only evidence against the physical nature of the studied objects, but also an interpretation on the lack of identification of more LMC age gap clusters.Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaWiley Blackwell Publishing, Inc2025-07info: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/11336/278764Piatti, Andres Eduardo; A hidden link in the LMC star cluster formation history; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 541; 7-2025; 3763-37710035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/541/4/3763/8213914info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/staf1242info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-01-14T12:56:37Zoai:ri.conicet.gov.ar:11336/278764instacron: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:34982026-01-14 12:56:37.839CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A hidden link in the LMC star cluster formation history
title A hidden link in the LMC star cluster formation history
spellingShingle A hidden link in the LMC star cluster formation history
Piatti, Andres Eduardo
cluster
title_short A hidden link in the LMC star cluster formation history
title_full A hidden link in the LMC star cluster formation history
title_fullStr A hidden link in the LMC star cluster formation history
title_full_unstemmed A hidden link in the LMC star cluster formation history
title_sort A hidden link in the LMC star cluster formation history
dc.creator.none.fl_str_mv Piatti, Andres Eduardo
author Piatti, Andres Eduardo
author_facet Piatti, Andres Eduardo
author_role author
dc.subject.none.fl_str_mv cluster
topic cluster
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The age distribution function of star clusters in the Large Magellanic Cloud (LMC) is known to present a feature called the cluster age gap, a period of time from ∼ 4 to 11 Gyr ago with a remarkable small number of clusters identified. In this work we performed an in-depth analysis of three recently catalogued age gap cluster candidates with the aim of confirming their physical nature. We used GEMINI@GMOS g, i pho- tometry centred on the objects to build colour-magnitude diagrams from which we recognised their main features. We also performed an automatic search of stellar over- densities using Gaussian mixture model techniques and analysed the corresponding colour-magnitude diagrams similarly as performed for the aforementioned candidates. The present GEMINI data sets would seem to discard any strong evidence of these object being real clusters, and rather support the possibility of the result of stellar density variations of the LMC field star distribution. These three objects, in addition to other 17 new identified candidates, are placed in the LMC outermost disc in a limited region toward the southwest from the LMC centre. They had embraced the possibility to answer the long-time conundrum about the absence of LMC age gap clusters. From an statistical approach, combined with the knowledge of the expected LMC age-metallicity relationship, and recent simulations of the interaction between the LMC and the Milky Way, we provide not only evidence against the physical nature of the studied objects, but also an interpretation on the lack of identification of more LMC age gap clusters.
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
description The age distribution function of star clusters in the Large Magellanic Cloud (LMC) is known to present a feature called the cluster age gap, a period of time from ∼ 4 to 11 Gyr ago with a remarkable small number of clusters identified. In this work we performed an in-depth analysis of three recently catalogued age gap cluster candidates with the aim of confirming their physical nature. We used GEMINI@GMOS g, i pho- tometry centred on the objects to build colour-magnitude diagrams from which we recognised their main features. We also performed an automatic search of stellar over- densities using Gaussian mixture model techniques and analysed the corresponding colour-magnitude diagrams similarly as performed for the aforementioned candidates. The present GEMINI data sets would seem to discard any strong evidence of these object being real clusters, and rather support the possibility of the result of stellar density variations of the LMC field star distribution. These three objects, in addition to other 17 new identified candidates, are placed in the LMC outermost disc in a limited region toward the southwest from the LMC centre. They had embraced the possibility to answer the long-time conundrum about the absence of LMC age gap clusters. From an statistical approach, combined with the knowledge of the expected LMC age-metallicity relationship, and recent simulations of the interaction between the LMC and the Milky Way, we provide not only evidence against the physical nature of the studied objects, but also an interpretation on the lack of identification of more LMC age gap clusters.
publishDate 2025
dc.date.none.fl_str_mv 2025-07
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/11336/278764
Piatti, Andres Eduardo; A hidden link in the LMC star cluster formation history; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 541; 7-2025; 3763-3771
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/278764
identifier_str_mv Piatti, Andres Eduardo; A hidden link in the LMC star cluster formation history; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 541; 7-2025; 3763-3771
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/url/https://academic.oup.com/mnras/article/541/4/3763/8213914
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/staf1242
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 Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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