Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses

Detalhes bibliográficos
Autor(a) principal: Bica, Eduardo Luiz Damiani
Data de Publicação: 2015
Outros Autores: Santiago, Basilio Xavier, Bonatto, Charles Jose, Dias, Rafael Augusto Garcia, Kerber, Leandro de Oliveira, Dias, Bruno Moreira de Souza, Barbuy, Beatriz, Balbinot, Eduardo
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/140442
Resumo: We obtained Southern Astrophysical Research telescope B and V photometry of 14 star clusters and two associations in the Bridge tidal structure connecting the Large and Small Magellanic Cloud (LMC and SMC). These objects are used to study the formation and evolution of star clusters and associations under tidal stresses from the Clouds. Typical star clusters in the Bridge are not richly populated and have in general relatively large diameters (≈30–35 pc), being larger than Galactic counterparts of similar age. Ages and other fundamental parameters are determined with field-star decontaminated photometry. A self-consistent approach is used to derive parameters for the most-populated sample cluster NGC 796 and two young CMD templates built with the remaining Bridge clusters. We find that the clusters are not coeval in the Bridge. They range from approximately a few Myr (still related to optical H II regions and WISE and Spitzer dust emission measurements) to about 100–200 Myr. The derived distance moduli for the Bridge objects (1h56m < α < 2h28m) suggests that the Bridge is a structure connecting the LMC farside in the east to the foreground of the SMC to the west. Most of the present clusters are part of the tidal dwarf candidate D 1, which is associated with an H I overdensity.We find further evidence that the studied part of the Bridge is evolving into a tidal dwarf galaxy, decoupling from the Bridge.
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spelling Bica, Eduardo Luiz DamianiSantiago, Basilio XavierBonatto, Charles JoseDias, Rafael Augusto GarciaKerber, Leandro de OliveiraDias, Bruno Moreira de SouzaBarbuy, BeatrizBalbinot, Eduardo2016-05-06T02:22:38Z20150035-8711http://hdl.handle.net/10183/140442000985423We obtained Southern Astrophysical Research telescope B and V photometry of 14 star clusters and two associations in the Bridge tidal structure connecting the Large and Small Magellanic Cloud (LMC and SMC). These objects are used to study the formation and evolution of star clusters and associations under tidal stresses from the Clouds. Typical star clusters in the Bridge are not richly populated and have in general relatively large diameters (≈30–35 pc), being larger than Galactic counterparts of similar age. Ages and other fundamental parameters are determined with field-star decontaminated photometry. A self-consistent approach is used to derive parameters for the most-populated sample cluster NGC 796 and two young CMD templates built with the remaining Bridge clusters. We find that the clusters are not coeval in the Bridge. They range from approximately a few Myr (still related to optical H II regions and WISE and Spitzer dust emission measurements) to about 100–200 Myr. The derived distance moduli for the Bridge objects (1h56m < α < 2h28m) suggests that the Bridge is a structure connecting the LMC farside in the east to the foreground of the SMC to the west. Most of the present clusters are part of the tidal dwarf candidate D 1, which is associated with an H I overdensity.We find further evidence that the studied part of the Bridge is evolving into a tidal dwarf galaxy, decoupling from the Bridge.application/pdfengMonthly notices of the Royal Astronomical Society. Oxford. Vol. 453, no. 3 (Nov. 2015), p. 3190-3202Nuvens de magalhaesAglomerados estelaresMagellanic cloudsGalaxies: star clusters: generalGalaxies: structureBridge over troubled gas : clusters and associations under the SMC and LMC tidal stressesEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000985423.pdf000985423.pdfTexto completo (inglês)application/pdf3766330http://www.lume.ufrgs.br/bitstream/10183/140442/1/000985423.pdf5a782d57ada63adb112bd0945115c9b0MD51TEXT000985423.pdf.txt000985423.pdf.txtExtracted Texttext/plain52945http://www.lume.ufrgs.br/bitstream/10183/140442/2/000985423.pdf.txt5b1258d178ef898271b33105d130c03fMD52THUMBNAIL000985423.pdf.jpg000985423.pdf.jpgGenerated Thumbnailimage/jpeg2112http://www.lume.ufrgs.br/bitstream/10183/140442/3/000985423.pdf.jpg4d24a092b9bc3daa888ca521ecdbdde2MD5310183/1404422023-07-02 03:41:44.958349oai:www.lume.ufrgs.br:10183/140442Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-02T06:41:44Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
title Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
spellingShingle Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
Bica, Eduardo Luiz Damiani
Nuvens de magalhaes
Aglomerados estelares
Magellanic clouds
Galaxies: star clusters: general
Galaxies: structure
title_short Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
title_full Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
title_fullStr Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
title_full_unstemmed Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
title_sort Bridge over troubled gas : clusters and associations under the SMC and LMC tidal stresses
author Bica, Eduardo Luiz Damiani
author_facet Bica, Eduardo Luiz Damiani
Santiago, Basilio Xavier
Bonatto, Charles Jose
Dias, Rafael Augusto Garcia
Kerber, Leandro de Oliveira
Dias, Bruno Moreira de Souza
Barbuy, Beatriz
Balbinot, Eduardo
author_role author
author2 Santiago, Basilio Xavier
Bonatto, Charles Jose
Dias, Rafael Augusto Garcia
Kerber, Leandro de Oliveira
Dias, Bruno Moreira de Souza
Barbuy, Beatriz
Balbinot, Eduardo
author2_role author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Bica, Eduardo Luiz Damiani
Santiago, Basilio Xavier
Bonatto, Charles Jose
Dias, Rafael Augusto Garcia
Kerber, Leandro de Oliveira
Dias, Bruno Moreira de Souza
Barbuy, Beatriz
Balbinot, Eduardo
dc.subject.por.fl_str_mv Nuvens de magalhaes
Aglomerados estelares
topic Nuvens de magalhaes
Aglomerados estelares
Magellanic clouds
Galaxies: star clusters: general
Galaxies: structure
dc.subject.eng.fl_str_mv Magellanic clouds
Galaxies: star clusters: general
Galaxies: structure
description We obtained Southern Astrophysical Research telescope B and V photometry of 14 star clusters and two associations in the Bridge tidal structure connecting the Large and Small Magellanic Cloud (LMC and SMC). These objects are used to study the formation and evolution of star clusters and associations under tidal stresses from the Clouds. Typical star clusters in the Bridge are not richly populated and have in general relatively large diameters (≈30–35 pc), being larger than Galactic counterparts of similar age. Ages and other fundamental parameters are determined with field-star decontaminated photometry. A self-consistent approach is used to derive parameters for the most-populated sample cluster NGC 796 and two young CMD templates built with the remaining Bridge clusters. We find that the clusters are not coeval in the Bridge. They range from approximately a few Myr (still related to optical H II regions and WISE and Spitzer dust emission measurements) to about 100–200 Myr. The derived distance moduli for the Bridge objects (1h56m < α < 2h28m) suggests that the Bridge is a structure connecting the LMC farside in the east to the foreground of the SMC to the west. Most of the present clusters are part of the tidal dwarf candidate D 1, which is associated with an H I overdensity.We find further evidence that the studied part of the Bridge is evolving into a tidal dwarf galaxy, decoupling from the Bridge.
publishDate 2015
dc.date.issued.fl_str_mv 2015
dc.date.accessioned.fl_str_mv 2016-05-06T02:22:38Z
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/140442
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dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv Monthly notices of the Royal Astronomical Society. Oxford. Vol. 453, no. 3 (Nov. 2015), p. 3190-3202
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