The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters

Autores
Oliveira, R. A. P.; Maia, F. F. S.; Barbuy, B.; Dias, B.; Santos Jr., J. F. C.; Souza, S. O.; Kerber, L.; Bica, E.; Sanmartim, D.; Quint, B.; Fraga, L.; Armond, T.; Minniti, D.; Parisi, Maria Celeste; Katime Santrich, O. J.; Angelo, M. S.; Pérez Villegas, A.; de Bórtoli, Bruno Javier
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The formation scenario of the Magellanic Bridge during an encounter between the Large and Small Magellanic Clouds ~200 Myr ago, as proposed by N-body models, would be imprinted in the chemical enrichment and kinematics of its stars and sites of ongoing star formation along its extension. We present an analysis of 33 Bridge star clusters using photometry obtained with the SOAR 4-m telescope equipped with adaptive optics for the VISCACHA survey. We performed a membership selection and derived self-consistent ages, metallicities, distances, and reddening values via statistical isochrone fitting, as well as tidal radii and integrated masses from structure analysis. Two groups are clearly detected: 13 well-studied clusters older than the Bridge, with 0.5-6.8 Gyr and [Fe/H]<−0.6 dex; and 15 clusters with <200 Myr and [Fe/H]>−0.5 dex, probably formed in situ. The old clusters follow the overall age and metallicity gradients of the SMC, whereas the younger ones are uniformly distributed along the Bridge. The main results are as follows: (i) we derive ages and metallicities for the first time for 9 and 18 clusters, respectively; (ii) we detect two metallicity dips in the age-metallicity relation of the Bridge at ~200 Myr and 1.5 Gyr ago for the first time, possibly chemical signatures of the formation of the Bridge and Magellanic Stream; (iii) we estimate a minimum stellar mass for the Bridge of 3-5 × 105 M⊙; (iv) we confirm that all the young Bridge clusters at RA<3h are metal-rich with [Fe/H]∼−0.4 dex.
Fil: Oliveira, R. A. P.. Universidade de Sao Paulo; Brasil
Fil: Maia, F. F. S.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Barbuy, B.. Universidade de Sao Paulo; Brasil
Fil: Dias, B.. Universidad de Tarapaca.; Chile
Fil: Santos Jr., J. F. C.. Departamento de Física - Ufmg; Brasil
Fil: Souza, S. O.. Universidade de Sao Paulo; Brasil
Fil: Kerber, L.. Universidade Estadual de Santa Cruz; Brasil
Fil: Bica, E.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Sanmartim, D.. Carnegie Institution For Science;
Fil: Quint, B.. Rubin Observatory; Estados Unidos
Fil: Fraga, L.. Laboratório Nacional de Astrofísica; Brasil
Fil: Armond, T.. Universidade Federal de São João Del-rei; Brasil
Fil: Minniti, D.. Universidad Andrés Bello; Chile
Fil: Parisi, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Katime Santrich, O. J.. Universidade Estadual de Santa Cruz; Brasil
Fil: Angelo, M. S.. Universidade Federal de Minas Gerais; Brasil
Fil: Pérez Villegas, A.. Universidad Nacional Autónoma de México; México
Fil: de Bórtoli, Bruno Javier. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Materia
MAGELLANIC CLOUDS
GALAXIES: EVOLUTION
GALAXIES: STAR CLUSTERS: GENERAL
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:11336/231624
Acceder
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network_name_str CONICET Digital (CONICET)
spelling The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clustersOliveira, R. A. P.Maia, F. F. S.Barbuy, B.Dias, B.Santos Jr., J. F. C.Souza, S. O.Kerber, L.Bica, E.Sanmartim, D.Quint, B.Fraga, L.Armond, T.Minniti, D.Parisi, Maria CelesteKatime Santrich, O. J.Angelo, M. S.Pérez Villegas, A.de Bórtoli, Bruno JavierMAGELLANIC CLOUDSGALAXIES: EVOLUTIONGALAXIES: STAR CLUSTERS: GENERALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The formation scenario of the Magellanic Bridge during an encounter between the Large and Small Magellanic Clouds ~200 Myr ago, as proposed by N-body models, would be imprinted in the chemical enrichment and kinematics of its stars and sites of ongoing star formation along its extension. We present an analysis of 33 Bridge star clusters using photometry obtained with the SOAR 4-m telescope equipped with adaptive optics for the VISCACHA survey. We performed a membership selection and derived self-consistent ages, metallicities, distances, and reddening values via statistical isochrone fitting, as well as tidal radii and integrated masses from structure analysis. Two groups are clearly detected: 13 well-studied clusters older than the Bridge, with 0.5-6.8 Gyr and [Fe/H]<−0.6 dex; and 15 clusters with <200 Myr and [Fe/H]>−0.5 dex, probably formed in situ. The old clusters follow the overall age and metallicity gradients of the SMC, whereas the younger ones are uniformly distributed along the Bridge. The main results are as follows: (i) we derive ages and metallicities for the first time for 9 and 18 clusters, respectively; (ii) we detect two metallicity dips in the age-metallicity relation of the Bridge at ~200 Myr and 1.5 Gyr ago for the first time, possibly chemical signatures of the formation of the Bridge and Magellanic Stream; (iii) we estimate a minimum stellar mass for the Bridge of 3-5 × 105 M⊙; (iv) we confirm that all the young Bridge clusters at RA<3h are metal-rich with [Fe/H]∼−0.4 dex.Fil: Oliveira, R. A. P.. Universidade de Sao Paulo; BrasilFil: Maia, F. F. S.. Universidade Federal do Rio de Janeiro; BrasilFil: Barbuy, B.. Universidade de Sao Paulo; BrasilFil: Dias, B.. Universidad de Tarapaca.; ChileFil: Santos Jr., J. F. C.. Departamento de Física - Ufmg; BrasilFil: Souza, S. O.. Universidade de Sao Paulo; BrasilFil: Kerber, L.. Universidade Estadual de Santa Cruz; BrasilFil: Bica, E.. Universidade Federal do Rio Grande do Sul; BrasilFil: Sanmartim, D.. Carnegie Institution For Science;Fil: Quint, B.. Rubin Observatory; Estados UnidosFil: Fraga, L.. Laboratório Nacional de Astrofísica; BrasilFil: Armond, T.. Universidade Federal de São João Del-rei; BrasilFil: Minniti, D.. Universidad Andrés Bello; ChileFil: Parisi, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Katime Santrich, O. J.. Universidade Estadual de Santa Cruz; BrasilFil: Angelo, M. S.. Universidade Federal de Minas Gerais; BrasilFil: Pérez Villegas, A.. Universidad Nacional Autónoma de México; MéxicoFil: de Bórtoli, Bruno Javier. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaOxford University Press2023-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/231624Oliveira, R. A. P.; Maia, F. F. S.; Barbuy, B.; Dias, B.; Santos Jr., J. F. C.; et al.; The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 524; 2; 9-2023; 2244-22611365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/524/2/2244/7199804info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad1827info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:45:26Zoai:ri.conicet.gov.ar:11336/231624instacron: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 11:45:26.991CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
title The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
spellingShingle The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
Oliveira, R. A. P.
MAGELLANIC CLOUDS
GALAXIES: EVOLUTION
GALAXIES: STAR CLUSTERS: GENERAL
title_short The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
title_full The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
title_fullStr The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
title_full_unstemmed The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
title_sort The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
dc.creator.none.fl_str_mv Oliveira, R. A. P.
Maia, F. F. S.
Barbuy, B.
Dias, B.
Santos Jr., J. F. C.
Souza, S. O.
Kerber, L.
Bica, E.
Sanmartim, D.
Quint, B.
Fraga, L.
Armond, T.
Minniti, D.
Parisi, Maria Celeste
Katime Santrich, O. J.
Angelo, M. S.
Pérez Villegas, A.
de Bórtoli, Bruno Javier
author Oliveira, R. A. P.
author_facet Oliveira, R. A. P.
Maia, F. F. S.
Barbuy, B.
Dias, B.
Santos Jr., J. F. C.
Souza, S. O.
Kerber, L.
Bica, E.
Sanmartim, D.
Quint, B.
Fraga, L.
Armond, T.
Minniti, D.
Parisi, Maria Celeste
Katime Santrich, O. J.
Angelo, M. S.
Pérez Villegas, A.
de Bórtoli, Bruno Javier
author_role author
author2 Maia, F. F. S.
Barbuy, B.
Dias, B.
Santos Jr., J. F. C.
Souza, S. O.
Kerber, L.
Bica, E.
Sanmartim, D.
Quint, B.
Fraga, L.
Armond, T.
Minniti, D.
Parisi, Maria Celeste
Katime Santrich, O. J.
Angelo, M. S.
Pérez Villegas, A.
de Bórtoli, Bruno Javier
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv MAGELLANIC CLOUDS
GALAXIES: EVOLUTION
GALAXIES: STAR CLUSTERS: GENERAL
topic MAGELLANIC CLOUDS
GALAXIES: EVOLUTION
GALAXIES: STAR CLUSTERS: GENERAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The formation scenario of the Magellanic Bridge during an encounter between the Large and Small Magellanic Clouds ~200 Myr ago, as proposed by N-body models, would be imprinted in the chemical enrichment and kinematics of its stars and sites of ongoing star formation along its extension. We present an analysis of 33 Bridge star clusters using photometry obtained with the SOAR 4-m telescope equipped with adaptive optics for the VISCACHA survey. We performed a membership selection and derived self-consistent ages, metallicities, distances, and reddening values via statistical isochrone fitting, as well as tidal radii and integrated masses from structure analysis. Two groups are clearly detected: 13 well-studied clusters older than the Bridge, with 0.5-6.8 Gyr and [Fe/H]<−0.6 dex; and 15 clusters with <200 Myr and [Fe/H]>−0.5 dex, probably formed in situ. The old clusters follow the overall age and metallicity gradients of the SMC, whereas the younger ones are uniformly distributed along the Bridge. The main results are as follows: (i) we derive ages and metallicities for the first time for 9 and 18 clusters, respectively; (ii) we detect two metallicity dips in the age-metallicity relation of the Bridge at ~200 Myr and 1.5 Gyr ago for the first time, possibly chemical signatures of the formation of the Bridge and Magellanic Stream; (iii) we estimate a minimum stellar mass for the Bridge of 3-5 × 105 M⊙; (iv) we confirm that all the young Bridge clusters at RA<3h are metal-rich with [Fe/H]∼−0.4 dex.
Fil: Oliveira, R. A. P.. Universidade de Sao Paulo; Brasil
Fil: Maia, F. F. S.. Universidade Federal do Rio de Janeiro; Brasil
Fil: Barbuy, B.. Universidade de Sao Paulo; Brasil
Fil: Dias, B.. Universidad de Tarapaca.; Chile
Fil: Santos Jr., J. F. C.. Departamento de Física - Ufmg; Brasil
Fil: Souza, S. O.. Universidade de Sao Paulo; Brasil
Fil: Kerber, L.. Universidade Estadual de Santa Cruz; Brasil
Fil: Bica, E.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Sanmartim, D.. Carnegie Institution For Science;
Fil: Quint, B.. Rubin Observatory; Estados Unidos
Fil: Fraga, L.. Laboratório Nacional de Astrofísica; Brasil
Fil: Armond, T.. Universidade Federal de São João Del-rei; Brasil
Fil: Minniti, D.. Universidad Andrés Bello; Chile
Fil: Parisi, Maria Celeste. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Katime Santrich, O. J.. Universidade Estadual de Santa Cruz; Brasil
Fil: Angelo, M. S.. Universidade Federal de Minas Gerais; Brasil
Fil: Pérez Villegas, A.. Universidad Nacional Autónoma de México; México
Fil: de Bórtoli, Bruno Javier. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
description The formation scenario of the Magellanic Bridge during an encounter between the Large and Small Magellanic Clouds ~200 Myr ago, as proposed by N-body models, would be imprinted in the chemical enrichment and kinematics of its stars and sites of ongoing star formation along its extension. We present an analysis of 33 Bridge star clusters using photometry obtained with the SOAR 4-m telescope equipped with adaptive optics for the VISCACHA survey. We performed a membership selection and derived self-consistent ages, metallicities, distances, and reddening values via statistical isochrone fitting, as well as tidal radii and integrated masses from structure analysis. Two groups are clearly detected: 13 well-studied clusters older than the Bridge, with 0.5-6.8 Gyr and [Fe/H]<−0.6 dex; and 15 clusters with <200 Myr and [Fe/H]>−0.5 dex, probably formed in situ. The old clusters follow the overall age and metallicity gradients of the SMC, whereas the younger ones are uniformly distributed along the Bridge. The main results are as follows: (i) we derive ages and metallicities for the first time for 9 and 18 clusters, respectively; (ii) we detect two metallicity dips in the age-metallicity relation of the Bridge at ~200 Myr and 1.5 Gyr ago for the first time, possibly chemical signatures of the formation of the Bridge and Magellanic Stream; (iii) we estimate a minimum stellar mass for the Bridge of 3-5 × 105 M⊙; (iv) we confirm that all the young Bridge clusters at RA<3h are metal-rich with [Fe/H]∼−0.4 dex.
publishDate 2023
dc.date.none.fl_str_mv 2023-09
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/11336/231624
Oliveira, R. A. P.; Maia, F. F. S.; Barbuy, B.; Dias, B.; Santos Jr., J. F. C.; et al.; The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 524; 2; 9-2023; 2244-2261
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/231624
identifier_str_mv Oliveira, R. A. P.; Maia, F. F. S.; Barbuy, B.; Dias, B.; Santos Jr., J. F. C.; et al.; The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 524; 2; 9-2023; 2244-2261
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://academic.oup.com/mnras/article/524/2/2244/7199804
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad1827
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
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score 12.982451

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