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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/278764
Ver los metadatos del registro completo
| id |
CONICETDig_bd4a6509ac9e1d59aba7b4f13c84da6b |
|---|---|
| oai_identifier_str |
oai:ri.conicet.gov.ar:11336/278764 |
| network_acronym_str |
CONICETDig |
| repository_id_str |
3498 |
| network_name_str |
CONICET Digital (CONICET) |
| 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 |
| _version_ |
1854322200303108096 |
| score |
13.113929 |