The VISCACHA survey - structure of outer MC star clusters

Autores
Santos Jr., João F. C.; Maia, F.; Dias, B.; Kerber, L.; Piatti, Andres Eduardo; Bica, Eduardo
Año de publicación
2020
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The Magellanic Clouds (MCs) constitute an interacting pair of galaxies influenced by the Milky Way gravitational field. Several studies have shown the effects of the changing tidal field on the structure of both Clouds. How the varying tidal field affects their stellar populations may be gauged via star clusters, where this connection may be more confidently stablished due to the accurate determination of the clusters astrophysical properties. Our objective is to perform an analysis of the structural parameters of 56 Large Magellanic Cloud (LMC) and 34 Small Magellanic Cloud (SMC) clusters located in the galaxies outskirts searching for signatures of tidal- dynamical effects eventually altering their evolution. To achieve our goal, AO assisted observations in BVI bands with the 4.1m SOAR telescope have been carried out, in the scope of the VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi HuguA) survey, in which an homogeneous, deep and high quality photometry is being produced. The structural parameters central stellar density, central surface brightness, core and tidal radius were obtained from King model fittings to the surface brightness and radial density profiles. By grouping clusters according to different regions we found that (i) the westernmost LMC clusters, the nearest ones to the SMC, have a larger dispersion of their core radius than those of the clusters located elsewhere; (ii) older clusters present a spread of core radius, similar to results from studies of inner MCs populous clusters.
Fil: Santos Jr., João F. C.. Universidade Federal de Minas Gerais; Brasil. Universidad de La Serena; Chile
Fil: Maia, F.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Dias, B.. Universidad Andrés Bello; Chile
Fil: Kerber, L.. Universidade Estadual de Santa Cruz; Brasil
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
Fil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; Brasil
XVI Latin American Regional Meeting International Astronomical Union
Antofagasta
Chile
Sociedad Chilena de Astronomía
Materia
CLUSTER
MAGELLANIC CLOUDS
CLOUDS
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:11336/213840
Acceder
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network_name_str CONICET Digital (CONICET)
spelling The VISCACHA survey - structure of outer MC star clustersSantos Jr., João F. C.Maia, F.Dias, B.Kerber, L.Piatti, Andres EduardoBica, EduardoCLUSTERMAGELLANIC CLOUDSCLOUDShttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1The Magellanic Clouds (MCs) constitute an interacting pair of galaxies influenced by the Milky Way gravitational field. Several studies have shown the effects of the changing tidal field on the structure of both Clouds. How the varying tidal field affects their stellar populations may be gauged via star clusters, where this connection may be more confidently stablished due to the accurate determination of the clusters astrophysical properties. Our objective is to perform an analysis of the structural parameters of 56 Large Magellanic Cloud (LMC) and 34 Small Magellanic Cloud (SMC) clusters located in the galaxies outskirts searching for signatures of tidal- dynamical effects eventually altering their evolution. To achieve our goal, AO assisted observations in BVI bands with the 4.1m SOAR telescope have been carried out, in the scope of the VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi HuguA) survey, in which an homogeneous, deep and high quality photometry is being produced. The structural parameters central stellar density, central surface brightness, core and tidal radius were obtained from King model fittings to the surface brightness and radial density profiles. By grouping clusters according to different regions we found that (i) the westernmost LMC clusters, the nearest ones to the SMC, have a larger dispersion of their core radius than those of the clusters located elsewhere; (ii) older clusters present a spread of core radius, similar to results from studies of inner MCs populous clusters.Fil: Santos Jr., João F. C.. Universidade Federal de Minas Gerais; Brasil. Universidad de La Serena; ChileFil: Maia, F.. Universidade Federal do Rio de Janeiro; BrasilFil: Dias, B.. Universidad Andrés Bello; ChileFil: Kerber, L.. Universidade Estadual de Santa Cruz; BrasilFil: 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; ArgentinaFil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; BrasilXVI Latin American Regional Meeting International Astronomical UnionAntofagastaChileSociedad Chilena de AstronomíaAsociación Argentina de AstronomíaFerrero Romero, J.Jimenez Bailon, E.Tissera, P. B.2020info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectReuniónJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/213840The VISCACHA survey - structure of outer MC star clusters; XVI Latin American Regional Meeting International Astronomical Union; Antofagasta; Chile; 2019; 98-981669-9521CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://astronomiaargentina.fcaglp.unlp.edu.ar/b61c/BAAA_61C_2020.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:57:52Zoai:ri.conicet.gov.ar:11336/213840instacron: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 11:57:52.821CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The VISCACHA survey - structure of outer MC star clusters
title The VISCACHA survey - structure of outer MC star clusters
spellingShingle The VISCACHA survey - structure of outer MC star clusters
Santos Jr., João F. C.
CLUSTER
MAGELLANIC CLOUDS
CLOUDS
title_short The VISCACHA survey - structure of outer MC star clusters
title_full The VISCACHA survey - structure of outer MC star clusters
title_fullStr The VISCACHA survey - structure of outer MC star clusters
title_full_unstemmed The VISCACHA survey - structure of outer MC star clusters
title_sort The VISCACHA survey - structure of outer MC star clusters
dc.creator.none.fl_str_mv Santos Jr., João F. C.
Maia, F.
Dias, B.
Kerber, L.
Piatti, Andres Eduardo
Bica, Eduardo
author Santos Jr., João F. C.
author_facet Santos Jr., João F. C.
Maia, F.
Dias, B.
Kerber, L.
Piatti, Andres Eduardo
Bica, Eduardo
author_role author
author2 Maia, F.
Dias, B.
Kerber, L.
Piatti, Andres Eduardo
Bica, Eduardo
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv Ferrero Romero, J.
Jimenez Bailon, E.
Tissera, P. B.
dc.subject.none.fl_str_mv CLUSTER
MAGELLANIC CLOUDS
CLOUDS
topic CLUSTER
MAGELLANIC CLOUDS
CLOUDS
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 Magellanic Clouds (MCs) constitute an interacting pair of galaxies influenced by the Milky Way gravitational field. Several studies have shown the effects of the changing tidal field on the structure of both Clouds. How the varying tidal field affects their stellar populations may be gauged via star clusters, where this connection may be more confidently stablished due to the accurate determination of the clusters astrophysical properties. Our objective is to perform an analysis of the structural parameters of 56 Large Magellanic Cloud (LMC) and 34 Small Magellanic Cloud (SMC) clusters located in the galaxies outskirts searching for signatures of tidal- dynamical effects eventually altering their evolution. To achieve our goal, AO assisted observations in BVI bands with the 4.1m SOAR telescope have been carried out, in the scope of the VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi HuguA) survey, in which an homogeneous, deep and high quality photometry is being produced. The structural parameters central stellar density, central surface brightness, core and tidal radius were obtained from King model fittings to the surface brightness and radial density profiles. By grouping clusters according to different regions we found that (i) the westernmost LMC clusters, the nearest ones to the SMC, have a larger dispersion of their core radius than those of the clusters located elsewhere; (ii) older clusters present a spread of core radius, similar to results from studies of inner MCs populous clusters.
Fil: Santos Jr., João F. C.. Universidade Federal de Minas Gerais; Brasil. Universidad de La Serena; Chile
Fil: Maia, F.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Dias, B.. Universidad Andrés Bello; Chile
Fil: Kerber, L.. Universidade Estadual de Santa Cruz; Brasil
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
Fil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; Brasil
XVI Latin American Regional Meeting International Astronomical Union
Antofagasta
Chile
Sociedad Chilena de Astronomía
description The Magellanic Clouds (MCs) constitute an interacting pair of galaxies influenced by the Milky Way gravitational field. Several studies have shown the effects of the changing tidal field on the structure of both Clouds. How the varying tidal field affects their stellar populations may be gauged via star clusters, where this connection may be more confidently stablished due to the accurate determination of the clusters astrophysical properties. Our objective is to perform an analysis of the structural parameters of 56 Large Magellanic Cloud (LMC) and 34 Small Magellanic Cloud (SMC) clusters located in the galaxies outskirts searching for signatures of tidal- dynamical effects eventually altering their evolution. To achieve our goal, AO assisted observations in BVI bands with the 4.1m SOAR telescope have been carried out, in the scope of the VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi HuguA) survey, in which an homogeneous, deep and high quality photometry is being produced. The structural parameters central stellar density, central surface brightness, core and tidal radius were obtained from King model fittings to the surface brightness and radial density profiles. By grouping clusters according to different regions we found that (i) the westernmost LMC clusters, the nearest ones to the SMC, have a larger dispersion of their core radius than those of the clusters located elsewhere; (ii) older clusters present a spread of core radius, similar to results from studies of inner MCs populous clusters.
publishDate 2020
dc.date.none.fl_str_mv 2020
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Reunión
Journal
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/213840
The VISCACHA survey - structure of outer MC star clusters; XVI Latin American Regional Meeting International Astronomical Union; Antofagasta; Chile; 2019; 98-98
1669-9521
CONICET Digital
CONICET
url http://hdl.handle.net/11336/213840
identifier_str_mv The VISCACHA survey - structure of outer MC star clusters; XVI Latin American Regional Meeting International Astronomical Union; Antofagasta; Chile; 2019; 98-98
1669-9521
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://astronomiaargentina.fcaglp.unlp.edu.ar/b61c/BAAA_61C_2020.pdf
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.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Asociación Argentina de Astronomía
publisher.none.fl_str_mv Asociación Argentina de Astronomía
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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