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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/231624
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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 Técnicas2025-09-29T10:15:13Zoai: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:34982025-09-29 10:15:13.344CONICET 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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1844614086792314880 |
score |
13.070432 |