The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1

Detalhes bibliográficos
Autor(a) principal: Soares, Jules Batista
Data de Publicação: 2003
Outros Autores: Bica, Eduardo Luiz Damiani
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/108024
Resumo: We employed J, H and Ks photometry from the 2MASS Point Source Catalogue to study the embedded star clusters in the nebulae vdB-RN 92 and Gy 3–7, which are located in the molecular cloud Canis Majoris R1. We employed colourcolour and colour-magnitudes diagrams together with theoretical pre-main sequence isochrones to derive their fundamental parameters. Ages are based on the fraction of stars with anomalous colours, supposedly of types Herbig AeBe and T Tauri. The vdB-RN 92 cluster has an age of 5–7 Myr and the Gy 3–7 cluster ≈2 Myr. The average reddening values are AV = 4.4 and AV = 6.3, respectively for vdB-RN 92 and Gy 3–7. The distance found for vdB-RN 92 was 1.5 kpc which is, within uncertainties, compatible with previous estimates for the complex. Gy 3–7 also appears to be related to the CMaR1 complex. We conclude that CMaR1 is a very active star-forming site, now with four star clusters in early evolutionary stages.
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spelling Soares, Jules BatistaBica, Eduardo Luiz Damiani2014-12-11T02:15:40Z20030004-6361http://hdl.handle.net/10183/108024000383462We employed J, H and Ks photometry from the 2MASS Point Source Catalogue to study the embedded star clusters in the nebulae vdB-RN 92 and Gy 3–7, which are located in the molecular cloud Canis Majoris R1. We employed colourcolour and colour-magnitudes diagrams together with theoretical pre-main sequence isochrones to derive their fundamental parameters. Ages are based on the fraction of stars with anomalous colours, supposedly of types Herbig AeBe and T Tauri. The vdB-RN 92 cluster has an age of 5–7 Myr and the Gy 3–7 cluster ≈2 Myr. The average reddening values are AV = 4.4 and AV = 6.3, respectively for vdB-RN 92 and Gy 3–7. The distance found for vdB-RN 92 was 1.5 kpc which is, within uncertainties, compatible with previous estimates for the complex. Gy 3–7 also appears to be related to the CMaR1 complex. We conclude that CMaR1 is a very active star-forming site, now with four star clusters in early evolutionary stages.application/pdfengAstronomy and astrophysics. Berlin. Vol. 404, no. 1 (June 2003), p. 217-222GalaxiaFormacao de estrelasEvolucao estelarFotometria estelarGalaxyOpen clusters and associationsGy 3–7, vdB-RN 92The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1Estrangeiroinfo: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:UFRGSORIGINAL000383462.pdf000383462.pdfTexto completo (inglês)application/pdf520479http://www.lume.ufrgs.br/bitstream/10183/108024/1/000383462.pdf8f93f17f2f4e2a1cdfce46e596f2b735MD51TEXT000383462.pdf.txt000383462.pdf.txtExtracted Texttext/plain22051http://www.lume.ufrgs.br/bitstream/10183/108024/2/000383462.pdf.txt36d48f1618473f59f1e74a4dc2c28aefMD52THUMBNAIL000383462.pdf.jpg000383462.pdf.jpgGenerated Thumbnailimage/jpeg1919http://www.lume.ufrgs.br/bitstream/10183/108024/3/000383462.pdf.jpg6537816f0815f0f5af2a4f017f638aa7MD5310183/1080242024-04-12 06:21:04.416542oai:www.lume.ufrgs.br:10183/108024Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-04-12T09:21:04Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
title The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
spellingShingle The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
Soares, Jules Batista
Galaxia
Formacao de estrelas
Evolucao estelar
Fotometria estelar
Galaxy
Open clusters and associations
Gy 3–7, vdB-RN 92
title_short The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
title_full The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
title_fullStr The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
title_full_unstemmed The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
title_sort The embedded star clysters in the nebulae vdB-RN 92 and Gy 3-7 in Canis Majoris R1
author Soares, Jules Batista
author_facet Soares, Jules Batista
Bica, Eduardo Luiz Damiani
author_role author
author2 Bica, Eduardo Luiz Damiani
author2_role author
dc.contributor.author.fl_str_mv Soares, Jules Batista
Bica, Eduardo Luiz Damiani
dc.subject.por.fl_str_mv Galaxia
Formacao de estrelas
Evolucao estelar
Fotometria estelar
topic Galaxia
Formacao de estrelas
Evolucao estelar
Fotometria estelar
Galaxy
Open clusters and associations
Gy 3–7, vdB-RN 92
dc.subject.eng.fl_str_mv Galaxy
Open clusters and associations
Gy 3–7, vdB-RN 92
description We employed J, H and Ks photometry from the 2MASS Point Source Catalogue to study the embedded star clusters in the nebulae vdB-RN 92 and Gy 3–7, which are located in the molecular cloud Canis Majoris R1. We employed colourcolour and colour-magnitudes diagrams together with theoretical pre-main sequence isochrones to derive their fundamental parameters. Ages are based on the fraction of stars with anomalous colours, supposedly of types Herbig AeBe and T Tauri. The vdB-RN 92 cluster has an age of 5–7 Myr and the Gy 3–7 cluster ≈2 Myr. The average reddening values are AV = 4.4 and AV = 6.3, respectively for vdB-RN 92 and Gy 3–7. The distance found for vdB-RN 92 was 1.5 kpc which is, within uncertainties, compatible with previous estimates for the complex. Gy 3–7 also appears to be related to the CMaR1 complex. We conclude that CMaR1 is a very active star-forming site, now with four star clusters in early evolutionary stages.
publishDate 2003
dc.date.issued.fl_str_mv 2003
dc.date.accessioned.fl_str_mv 2014-12-11T02:15:40Z
dc.type.driver.fl_str_mv Estrangeiro
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status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/108024
dc.identifier.issn.pt_BR.fl_str_mv 0004-6361
dc.identifier.nrb.pt_BR.fl_str_mv 000383462
identifier_str_mv 0004-6361
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url http://hdl.handle.net/10183/108024
dc.language.iso.fl_str_mv eng
language eng
dc.relation.ispartof.pt_BR.fl_str_mv Astronomy and astrophysics. Berlin. Vol. 404, no. 1 (June 2003), p. 217-222
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
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reponame_str Repositório Institucional da UFRGS
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