Characterizing star cluster formation with WISE : 652 newly found star clusters and candidates
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | , |
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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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 info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
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 |
identifier_str_mv |
0035-8711 000985645 |
url |
http://hdl.handle.net/10183/140348 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
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 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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application/pdf |
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