Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates

Detalhes bibliográficos
Autor(a) principal: Camargo, Denilso da Silva
Data de Publicação: 2016
Outros Autores: Bica, Eduardo Luiz Damiani, Bonatto, Charles Jose
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/140348
Resumo: We report the discovery of 652 star clusters, stellar groups and candidates in the Milky Way with Wide-field Infrared Survey Explorer (WISE). Most of the objects are projected close to Galactic plane and are embedded clusters. The present sample complements a similar study (Paper I) which provided 437 star clusters and alike. We find evidence that star formation processes span a wide range of sizes, from populous dense clusters to small compact embedded ones, sparse stellar groups or in relative isolation. The present list indicates multiple stellar generations during the embedded phase, with giant molecular clouds collapsing into several clumps composing an embedded cluster aggregate.We investigate the field star decontaminated colour–magnitude diagrams and radial density profiles of nine cluster candidates in the list, and derive their parameters, confirming them as embedded clusters.
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spelling Camargo, Denilso da SilvaBica, Eduardo Luiz DamianiBonatto, Charles Jose2016-05-06T02:21:47Z20160035-8711http://hdl.handle.net/10183/140348000985645We report the discovery of 652 star clusters, stellar groups and candidates in the Milky Way with Wide-field Infrared Survey Explorer (WISE). Most of the objects are projected close to Galactic plane and are embedded clusters. The present sample complements a similar study (Paper I) which provided 437 star clusters and alike. We find evidence that star formation processes span a wide range of sizes, from populous dense clusters to small compact embedded ones, sparse stellar groups or in relative isolation. The present list indicates multiple stellar generations during the embedded phase, with giant molecular clouds collapsing into several clumps composing an embedded cluster aggregate.We investigate the field star decontaminated colour–magnitude diagrams and radial density profiles of nine cluster candidates in the list, and derive their parameters, confirming them as embedded clusters.application/pdfengMonthly notices of the Royal Astronomical Society. Oxford. Vol. 455, no. 3 (Jan. 2016), p. 3126-3135Aglomerados estelaresFormacao de estrelasCataloguesGalaxy: discOpen clusters and associations: generalGalaxy: structureCharacterizing star cluster formation with WISE : 652 newly found star clusters and candidatesEstrangeiroinfo: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:UFRGSORIGINAL000985645.pdf000985645.pdfTexto completo (inglês)application/pdf11134726http://www.lume.ufrgs.br/bitstream/10183/140348/1/000985645.pdf8acc44e698abba8a4d7af0b10b6a10aaMD51TEXT000985645.pdf.txt000985645.pdf.txtExtracted Texttext/plain33777http://www.lume.ufrgs.br/bitstream/10183/140348/2/000985645.pdf.txtb1519e23e04915a19eec67641827ba6fMD52THUMBNAIL000985645.pdf.jpg000985645.pdf.jpgGenerated Thumbnailimage/jpeg2140http://www.lume.ufrgs.br/bitstream/10183/140348/3/000985645.pdf.jpg89cb6a73afa12eae509322da85f16d0dMD5310183/1403482023-07-15 03:28:09.952564oai:www.lume.ufrgs.br:10183/140348Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-15T06:28:09Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
title Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
spellingShingle Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
Camargo, Denilso da Silva
Aglomerados estelares
Formacao de estrelas
Catalogues
Galaxy: disc
Open clusters and associations: general
Galaxy: structure
title_short Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
title_full Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
title_fullStr Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
title_full_unstemmed Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
title_sort Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
author Camargo, Denilso da Silva
author_facet Camargo, Denilso da Silva
Bica, Eduardo Luiz Damiani
Bonatto, Charles Jose
author_role author
author2 Bica, Eduardo Luiz Damiani
Bonatto, Charles Jose
author2_role author
author
dc.contributor.author.fl_str_mv Camargo, Denilso da Silva
Bica, Eduardo Luiz Damiani
Bonatto, Charles Jose
dc.subject.por.fl_str_mv Aglomerados estelares
Formacao de estrelas
topic Aglomerados estelares
Formacao de estrelas
Catalogues
Galaxy: disc
Open clusters and associations: general
Galaxy: structure
dc.subject.eng.fl_str_mv Catalogues
Galaxy: disc
Open clusters and associations: general
Galaxy: structure
description We report the discovery of 652 star clusters, stellar groups and candidates in the Milky Way with Wide-field Infrared Survey Explorer (WISE). Most of the objects are projected close to Galactic plane and are embedded clusters. The present sample complements a similar study (Paper I) which provided 437 star clusters and alike. We find evidence that star formation processes span a wide range of sizes, from populous dense clusters to small compact embedded ones, sparse stellar groups or in relative isolation. The present list indicates multiple stellar generations during the embedded phase, with giant molecular clouds collapsing into several clumps composing an embedded cluster aggregate.We investigate the field star decontaminated colour–magnitude diagrams and radial density profiles of nine cluster candidates in the list, and derive their parameters, confirming them as embedded clusters.
publishDate 2016
dc.date.accessioned.fl_str_mv 2016-05-06T02:21:47Z
dc.date.issued.fl_str_mv 2016
dc.type.driver.fl_str_mv Estrangeiro
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/140348
dc.identifier.issn.pt_BR.fl_str_mv 0035-8711
dc.identifier.nrb.pt_BR.fl_str_mv 000985645
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000985645
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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. 455, no. 3 (Jan. 2016), p. 3126-3135
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