The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery

Autores
Santos, Joao F. C.; Maia, Francisco; Dias, Bruno; de O. Kerber, Leandro; Piatti, Andres Eduardo; Bica, Eduardo; Angelo, Mateus S.; Minniti, Dante; Pérez Villegas, Angeles; Roman Lopes, Alexandre; Westera, Pieter; Fraga, Luciano; Quint, Bruno; Sanmartim, David
Año de publicación
2020
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters’ stellar density and surface brightness profiles were built from deep, AO assisted optical images, and uniform analysis techniques. The structural parameters were obtained from King and Elson et al. model fittings. Integrated magnitudes and masses (for a subsample) are also provided. The sample contains mostly low surface brightness clusters with distances between 4.5 and 6.5 kpc and between 1 and 6.5 kpc from the LMC and SMC centres, respectively. We analysed their spatial distribution and structural properties, comparing them with those of inner clusters. Half-light and Jacobi radii were estimated, allowing an evaluation of the Roche volume tidal filling. We found that: (i) for both MCs, the tidal radii are on average larger than those of inner clusters; (ii) the core radii dispersion tends to be greater for LMC clusters located towards the southwest, with position angles of ∼200 degrees and about ∼5 degrees from the LMC centre, i.e., those LMC clusters nearer to the SMC; (iii) the analysis of clusters with ages available revealed that the core radius evolution is similar to the one of inner clusters; (iv) Roche volumes are overfilled for SMC clusters with galactocentric distances closer than 3 kpc.
Fil: Santos, Joao F. C.. Universidad de La Serena; Chile. Universidade Federal de Minas Gerais; Brasil
Fil: Maia, Francisco. Universidade Federal do Rio de Janeiro; Brasil
Fil: Dias, Bruno. Millennium Institute of Astrophysics; Chile. Universidad Andrés Bello; Chile
Fil: de O. Kerber, Leandro. Universidade Estadual de Santa Cruz; Brasil
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Angelo, Mateus S.. Centro Federal de Educacao Tecnológica de Minas Gerais; Brasil
Fil: Minniti, Dante. Universidad Andrés Bello; Chile. Millennium Institute of Astrophysics; Chile. Vatican Observatory; Italia
Fil: Pérez Villegas, Angeles. Universidade de Sao Paulo; Brasil
Fil: Roman Lopes, Alexandre. Universidad de La Serena; Chile
Fil: Westera, Pieter. Universidad Federal Do Abc; Brasil
Fil: Fraga, Luciano. Laboratorio Nacional de Astrofísica; Brasil
Fil: Quint, Bruno. Gemini Observatory; Chile
Fil: Sanmartim, David. Carnegie Institution of Washington; Chile
Materia
CLUSTER
GALAXIES: STAR CLUSTERS: GENERAL
Galaxies: interactions
Surveys
Galaxies: photometry
Galaxies: structure
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:11336/139454
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/139454
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds peripherySantos, Joao F. C.Maia, FranciscoDias, Brunode O. Kerber, LeandroPiatti, Andres EduardoBica, EduardoAngelo, Mateus S.Minniti, DantePérez Villegas, AngelesRoman Lopes, AlexandreWestera, PieterFraga, LucianoQuint, BrunoSanmartim, DavidCLUSTERGALAXIES: STAR CLUSTERS: GENERALGalaxies: interactionsSurveysGalaxies: photometryGalaxies: structurehttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters’ stellar density and surface brightness profiles were built from deep, AO assisted optical images, and uniform analysis techniques. The structural parameters were obtained from King and Elson et al. model fittings. Integrated magnitudes and masses (for a subsample) are also provided. The sample contains mostly low surface brightness clusters with distances between 4.5 and 6.5 kpc and between 1 and 6.5 kpc from the LMC and SMC centres, respectively. We analysed their spatial distribution and structural properties, comparing them with those of inner clusters. Half-light and Jacobi radii were estimated, allowing an evaluation of the Roche volume tidal filling. We found that: (i) for both MCs, the tidal radii are on average larger than those of inner clusters; (ii) the core radii dispersion tends to be greater for LMC clusters located towards the southwest, with position angles of ∼200 degrees and about ∼5 degrees from the LMC centre, i.e., those LMC clusters nearer to the SMC; (iii) the analysis of clusters with ages available revealed that the core radius evolution is similar to the one of inner clusters; (iv) Roche volumes are overfilled for SMC clusters with galactocentric distances closer than 3 kpc.Fil: Santos, Joao F. C.. Universidad de La Serena; Chile. Universidade Federal de Minas Gerais; BrasilFil: Maia, Francisco. Universidade Federal do Rio de Janeiro; BrasilFil: Dias, Bruno. Millennium Institute of Astrophysics; Chile. Universidad Andrés Bello; ChileFil: de O. Kerber, Leandro. Universidade Estadual de Santa Cruz; BrasilFil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; BrasilFil: Angelo, Mateus S.. Centro Federal de Educacao Tecnológica de Minas Gerais; BrasilFil: Minniti, Dante. Universidad Andrés Bello; Chile. Millennium Institute of Astrophysics; Chile. Vatican Observatory; ItaliaFil: Pérez Villegas, Angeles. Universidade de Sao Paulo; BrasilFil: Roman Lopes, Alexandre. Universidad de La Serena; ChileFil: Westera, Pieter. Universidad Federal Do Abc; BrasilFil: Fraga, Luciano. Laboratorio Nacional de Astrofísica; BrasilFil: Quint, Bruno. Gemini Observatory; ChileFil: Sanmartim, David. Carnegie Institution of Washington; ChileOxford University Press2020-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/139454Santos, Joao F. C.; Maia, Francisco; Dias, Bruno; de O. Kerber, Leandro; Piatti, Andres Eduardo; et al.; The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 498; 8-2020; 205-2220035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2008.04399info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:52:23Zoai:ri.conicet.gov.ar:11336/139454instacron: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 09:52:23.965CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
title The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
spellingShingle The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
Santos, Joao F. C.
CLUSTER
GALAXIES: STAR CLUSTERS: GENERAL
Galaxies: interactions
Surveys
Galaxies: photometry
Galaxies: structure
title_short The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
title_full The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
title_fullStr The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
title_full_unstemmed The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
title_sort The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery
dc.creator.none.fl_str_mv Santos, Joao F. C.
Maia, Francisco
Dias, Bruno
de O. Kerber, Leandro
Piatti, Andres Eduardo
Bica, Eduardo
Angelo, Mateus S.
Minniti, Dante
Pérez Villegas, Angeles
Roman Lopes, Alexandre
Westera, Pieter
Fraga, Luciano
Quint, Bruno
Sanmartim, David
author Santos, Joao F. C.
author_facet Santos, Joao F. C.
Maia, Francisco
Dias, Bruno
de O. Kerber, Leandro
Piatti, Andres Eduardo
Bica, Eduardo
Angelo, Mateus S.
Minniti, Dante
Pérez Villegas, Angeles
Roman Lopes, Alexandre
Westera, Pieter
Fraga, Luciano
Quint, Bruno
Sanmartim, David
author_role author
author2 Maia, Francisco
Dias, Bruno
de O. Kerber, Leandro
Piatti, Andres Eduardo
Bica, Eduardo
Angelo, Mateus S.
Minniti, Dante
Pérez Villegas, Angeles
Roman Lopes, Alexandre
Westera, Pieter
Fraga, Luciano
Quint, Bruno
Sanmartim, David
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv CLUSTER
GALAXIES: STAR CLUSTERS: GENERAL
Galaxies: interactions
Surveys
Galaxies: photometry
Galaxies: structure
topic CLUSTER
GALAXIES: STAR CLUSTERS: GENERAL
Galaxies: interactions
Surveys
Galaxies: photometry
Galaxies: structure
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters’ stellar density and surface brightness profiles were built from deep, AO assisted optical images, and uniform analysis techniques. The structural parameters were obtained from King and Elson et al. model fittings. Integrated magnitudes and masses (for a subsample) are also provided. The sample contains mostly low surface brightness clusters with distances between 4.5 and 6.5 kpc and between 1 and 6.5 kpc from the LMC and SMC centres, respectively. We analysed their spatial distribution and structural properties, comparing them with those of inner clusters. Half-light and Jacobi radii were estimated, allowing an evaluation of the Roche volume tidal filling. We found that: (i) for both MCs, the tidal radii are on average larger than those of inner clusters; (ii) the core radii dispersion tends to be greater for LMC clusters located towards the southwest, with position angles of ∼200 degrees and about ∼5 degrees from the LMC centre, i.e., those LMC clusters nearer to the SMC; (iii) the analysis of clusters with ages available revealed that the core radius evolution is similar to the one of inner clusters; (iv) Roche volumes are overfilled for SMC clusters with galactocentric distances closer than 3 kpc.
Fil: Santos, Joao F. C.. Universidad de La Serena; Chile. Universidade Federal de Minas Gerais; Brasil
Fil: Maia, Francisco. Universidade Federal do Rio de Janeiro; Brasil
Fil: Dias, Bruno. Millennium Institute of Astrophysics; Chile. Universidad Andrés Bello; Chile
Fil: de O. Kerber, Leandro. Universidade Estadual de Santa Cruz; Brasil
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Bica, Eduardo. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Angelo, Mateus S.. Centro Federal de Educacao Tecnológica de Minas Gerais; Brasil
Fil: Minniti, Dante. Universidad Andrés Bello; Chile. Millennium Institute of Astrophysics; Chile. Vatican Observatory; Italia
Fil: Pérez Villegas, Angeles. Universidade de Sao Paulo; Brasil
Fil: Roman Lopes, Alexandre. Universidad de La Serena; Chile
Fil: Westera, Pieter. Universidad Federal Do Abc; Brasil
Fil: Fraga, Luciano. Laboratorio Nacional de Astrofísica; Brasil
Fil: Quint, Bruno. Gemini Observatory; Chile
Fil: Sanmartim, David. Carnegie Institution of Washington; Chile
description We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters’ stellar density and surface brightness profiles were built from deep, AO assisted optical images, and uniform analysis techniques. The structural parameters were obtained from King and Elson et al. model fittings. Integrated magnitudes and masses (for a subsample) are also provided. The sample contains mostly low surface brightness clusters with distances between 4.5 and 6.5 kpc and between 1 and 6.5 kpc from the LMC and SMC centres, respectively. We analysed their spatial distribution and structural properties, comparing them with those of inner clusters. Half-light and Jacobi radii were estimated, allowing an evaluation of the Roche volume tidal filling. We found that: (i) for both MCs, the tidal radii are on average larger than those of inner clusters; (ii) the core radii dispersion tends to be greater for LMC clusters located towards the southwest, with position angles of ∼200 degrees and about ∼5 degrees from the LMC centre, i.e., those LMC clusters nearer to the SMC; (iii) the analysis of clusters with ages available revealed that the core radius evolution is similar to the one of inner clusters; (iv) Roche volumes are overfilled for SMC clusters with galactocentric distances closer than 3 kpc.
publishDate 2020
dc.date.none.fl_str_mv 2020-08
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/11336/139454
Santos, Joao F. C.; Maia, Francisco; Dias, Bruno; de O. Kerber, Leandro; Piatti, Andres Eduardo; et al.; The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 498; 8-2020; 205-222
0035-8711
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/139454
identifier_str_mv Santos, Joao F. C.; Maia, Francisco; Dias, Bruno; de O. Kerber, Leandro; Piatti, Andres Eduardo; et al.; The Viscacha survey - II: Structure of star clusters in the Magellanic Clouds periphery; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 498; 8-2020; 205-222
0035-8711
1365-2966
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://arxiv.org/abs/2008.04399
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.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
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_ 1844613607329890304
score 13.070432

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