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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/213840
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:25:09Zoai: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:34982025-09-29 10:25:10.165CONICET 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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13.070432 |