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Please use this identifier to cite or link to this item: http://hdl.handle.net/1843/64330
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dc.creatorBruno Moreira de Souza Diaspt_BR
dc.creatorBeatriz Leonor Silveira Barbuypt_BR
dc.creatorEduardo Luiz Damiani Bicapt_BR
dc.creatorDouglas Paul Geislerpt_BR
dc.creatorLeandro de Oliveira Kerberpt_BR
dc.creatorMaria de Los Angeles Perez Villegaspt_BR
dc.creatorBruno Corrêa Quintpt_BR
dc.creatorDavid Sanmartimpt_BR
dc.creatorJoão Francisco Coelho dos Santos Juniorpt_BR
dc.creatorPieter Willem Westerapt_BR
dc.creatorMateus de Souza Angelopt_BR
dc.creatorRaphael Augusto Pereira de Oliveirapt_BR
dc.creatorFrancisco Ferreira de Souza Maiapt_BR
dc.creatorMaría Celeste Parisipt_BR
dc.creatorBruno Javier De Bórtolipt_BR
dc.creatorStefano Oliveira de Souzapt_BR
dc.creatorOrlando José Katime Santrichpt_BR
dc.creatorLilia Patricia Bassinopt_BR
dc.date.accessioned2024-02-20T17:25:10Z-
dc.date.available2024-02-20T17:25:10Z-
dc.date.issued2021-
dc.citation.volume647pt_BR
dc.citation.spage1pt_BR
dc.citation.epage10pt_BR
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202040015pt_BR
dc.identifier.issn1432-0746pt_BR
dc.identifier.urihttp://hdl.handle.net/1843/64330-
dc.description.resumoCONTEXT. The interactions between the Small and Large Magellanic Clouds (SMC and LMC) created the Magellanic Bridge; a stream of gas and stars pulled out of the SMC towards the LMC about 150 Myr ago. The tidal counterpart of this structure, which should include a trailing arm, has been predicted by models but no compelling observational evidence has confirmed the Counter-Bridge so far. AIMS. The main goal of this work is to find the stellar counterpart of the Magellanic Bridge and Counter-Bridge. We use star clusters in the SMC outskirts as they provide a 6D phase-space vector, age, and metallicity which help characterise the outskirts of the SMC. METHODS. Distances, ages, and photometric metallicities were derived from fitting isochrones to the colour-magnitude diagrams from the VISCACHA survey. Radial velocities and spectroscopic metallicities were derived from the spectroscopic follow-up using GMOS in the CaII triplet region. RESULTS. Among the seven clusters analysed in this work, five belong to the Magellanic Bridge, one belongs to the Counter-Bridge, and the other belongs to the transition region. CONCLUSIONS. The existence of the tidal counterpart of the Magellanic Bridge is evidenced by star clusters. The stellar component of the Magellanic Bridge and Counter-Bridge are confirmed in the SMC outskirts. These results are an important constraint for models that seek to reconstruct the history of the orbit and interactions between the LMC and SMC as well as constrain their future interaction including with the Milky Way.pt_BR
dc.description.sponsorshipCAPES - Coordenação de Aperfeiçoamento de Pessoal de Nível Superiorpt_BR
dc.description.sponsorshipFAPESP - Fundação de Amparo à Pesquisa do Estado de São Paulopt_BR
dc.format.mimetypepdfpt_BR
dc.languageengpt_BR
dc.publisherUniversidade Federal de Minas Geraispt_BR
dc.publisher.countryBrasilpt_BR
dc.publisher.departmentICX - DEPARTAMENTO DE FÍSICApt_BR
dc.publisher.initialsUFMGpt_BR
dc.relation.ispartofA&A-
dc.rightsAcesso Abertopt_BR
dc.subjectMagellanic cloudspt_BR
dc.subjectStar clusterspt_BR
dc.subjectGalaxiespt_BR
dc.subject.otherAglomerado de estrelaspt_BR
dc.subject.otherGaláxiaspt_BR
dc.titleThe VISCACHA survey - III. Star clusters counterpart of the Magellanic bridge and counter-bridge in 8Dpt_BR
dc.typeArtigo de Periódicopt_BR
dc.url.externahttps://www.aanda.org/articles/aa/full_html/2021/03/aa40015-20/aa40015-20.htmlpt_BR
dc.identifier.orcidhttps://orcid.org/0000-0003-4254-7111pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0001-9264-4417pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-7435-8748pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-1557-3560pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-9238-9521pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0003-1794-6356pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0003-3379-994Xpt_BR
dc.identifier.orcidhttps://orcid.org/0000-0001-6138-0674pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-4778-9243pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-2569-4032pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0001-9382-3986pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-1005-3080pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0001-8052-969Xpt_BR
dc.identifier.orcidhttps://orcid.org/0000-0003-0439-2331pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0003-3152-6497pt_BR
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