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dc.contributor.authorCamargo, Denilso da Silvapt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorBonatto, Charles Josept_BR
dc.date.accessioned2016-05-06T02:21:47Zpt_BR
dc.date.issued2016pt_BR
dc.identifier.issn0035-8711pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/140348pt_BR
dc.description.abstractWe 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.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofMonthly notices of the Royal Astronomical Society. Oxford. Vol. 455, no. 3 (Jan. 2016), p. 3126-3135pt_BR
dc.rightsOpen Accessen
dc.subjectCataloguesen
dc.subjectAglomerados estelarespt_BR
dc.subjectFormacao de estrelaspt_BR
dc.subjectGalaxy: discen
dc.subjectOpen clusters and associations: generalen
dc.subjectGalaxy: structureen
dc.titleCharacterizing star cluster formation with WISE : 652 newly found star clusters and candidatespt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000985645pt_BR
dc.type.originEstrangeiropt_BR


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