Astrophysical parameters of 14 open clusters projected close to the Galactic plane
Autor(a) principal: | |
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Data de Publicação: | 2009 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/99263 |
Resumo: | Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open clusters (OCs) projected close to the Galactic plane are derived with 2MASS photometry. The OCs are Be 63, Be 84, Cz 6, Cz 7, Cz 12, Ru 141, Ru 144, Ru 172, FSR101, FSR1430, FSR1471, FSR162, FSR178, and FSR198. The OCs Be 63, Be 84, Ru 141, Ru 144, and Ru 172 are studied in more detail than in previous works, while the others have astrophysical parameters derived for the first time. Methods. We analyse the colour−magnitude diagrams (CMDs) and stellar radial density profiles (RDPs) built after field-star decontamination and colour-magnitude filtered photometry. Field-star decontamination is applied to uncover the cluster’s intrinsic CMD morphology, and colour−magnitude filters are used to isolate stars with a high probability of being cluster members in view of structural analyses. Results. The open clusters of the sample are located at d = 1.6−7.1 kpc from the Sun and at Galactocentric distances 5.5−11.8 kpc, with age in the range 10 Myr to 1.5 Gyr and reddening E(B−V) in the range 0.19−2.56 mag. The core and cluster radii are in the range 0.27−1.88 pc and 2.2−11.27 pc, respectively. Cz 6 and FSR198 are the youngest OCs of this sample, with a population of pre-main sequence (PMS) stars, while FSR 178 is the oldest cluster. |
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Camargo, Denilso da SilvaBonatto, Charles JoseBica, Eduardo Luiz Damiani2014-08-08T02:07:03Z20090004-6361http://hdl.handle.net/10183/99263000827391Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open clusters (OCs) projected close to the Galactic plane are derived with 2MASS photometry. The OCs are Be 63, Be 84, Cz 6, Cz 7, Cz 12, Ru 141, Ru 144, Ru 172, FSR101, FSR1430, FSR1471, FSR162, FSR178, and FSR198. The OCs Be 63, Be 84, Ru 141, Ru 144, and Ru 172 are studied in more detail than in previous works, while the others have astrophysical parameters derived for the first time. Methods. We analyse the colour−magnitude diagrams (CMDs) and stellar radial density profiles (RDPs) built after field-star decontamination and colour-magnitude filtered photometry. Field-star decontamination is applied to uncover the cluster’s intrinsic CMD morphology, and colour−magnitude filters are used to isolate stars with a high probability of being cluster members in view of structural analyses. Results. The open clusters of the sample are located at d = 1.6−7.1 kpc from the Sun and at Galactocentric distances 5.5−11.8 kpc, with age in the range 10 Myr to 1.5 Gyr and reddening E(B−V) in the range 0.19−2.56 mag. The core and cluster radii are in the range 0.27−1.88 pc and 2.2−11.27 pc, respectively. Cz 6 and FSR198 are the youngest OCs of this sample, with a population of pre-main sequence (PMS) stars, while FSR 178 is the oldest cluster.application/pdfengAstronomy and astrophysics. Les Ulis. Vol. 508, no. 1 (Dec. 2009), p. 211-220Aglomerados abertos e associaçõesAglomerados estelaresEstrutura estelarFotometria estelarOpen clusters and associations: general – –Galaxy: stellar contentGalaxy: structureAstrophysical parameters of 14 open clusters projected close to the Galactic planeEstrangeiroinfo: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:UFRGSORIGINAL000827391.pdf000827391.pdfTexto completo (inglês)application/pdf760349http://www.lume.ufrgs.br/bitstream/10183/99263/1/000827391.pdffcef8ed942328251835b20b0c65a8467MD51TEXT000827391.pdf.txt000827391.pdf.txtExtracted Texttext/plain44616http://www.lume.ufrgs.br/bitstream/10183/99263/2/000827391.pdf.txt6230f290b4258ecfe2b007db84f70669MD52THUMBNAIL000827391.pdf.jpg000827391.pdf.jpgGenerated Thumbnailimage/jpeg2020http://www.lume.ufrgs.br/bitstream/10183/99263/3/000827391.pdf.jpgad2ef25c3f77264b131d5392ad4a5fdfMD5310183/992632023-07-15 03:28:46.810745oai:www.lume.ufrgs.br:10183/99263Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-15T06:28:46Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
title |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
spellingShingle |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane Camargo, Denilso da Silva Aglomerados abertos e associações Aglomerados estelares Estrutura estelar Fotometria estelar Open clusters and associations: general – – Galaxy: stellar content Galaxy: structure |
title_short |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
title_full |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
title_fullStr |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
title_full_unstemmed |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
title_sort |
Astrophysical parameters of 14 open clusters projected close to the Galactic plane |
author |
Camargo, Denilso da Silva |
author_facet |
Camargo, Denilso da Silva Bonatto, Charles Jose Bica, Eduardo Luiz Damiani |
author_role |
author |
author2 |
Bonatto, Charles Jose Bica, Eduardo Luiz Damiani |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Camargo, Denilso da Silva Bonatto, Charles Jose Bica, Eduardo Luiz Damiani |
dc.subject.por.fl_str_mv |
Aglomerados abertos e associações Aglomerados estelares Estrutura estelar Fotometria estelar |
topic |
Aglomerados abertos e associações Aglomerados estelares Estrutura estelar Fotometria estelar Open clusters and associations: general – – Galaxy: stellar content Galaxy: structure |
dc.subject.eng.fl_str_mv |
Open clusters and associations: general – – Galaxy: stellar content Galaxy: structure |
description |
Aims. Astrophysical parameters (age, reddening, distance, core and cluster radii) of 14 open clusters (OCs) projected close to the Galactic plane are derived with 2MASS photometry. The OCs are Be 63, Be 84, Cz 6, Cz 7, Cz 12, Ru 141, Ru 144, Ru 172, FSR101, FSR1430, FSR1471, FSR162, FSR178, and FSR198. The OCs Be 63, Be 84, Ru 141, Ru 144, and Ru 172 are studied in more detail than in previous works, while the others have astrophysical parameters derived for the first time. Methods. We analyse the colour−magnitude diagrams (CMDs) and stellar radial density profiles (RDPs) built after field-star decontamination and colour-magnitude filtered photometry. Field-star decontamination is applied to uncover the cluster’s intrinsic CMD morphology, and colour−magnitude filters are used to isolate stars with a high probability of being cluster members in view of structural analyses. Results. The open clusters of the sample are located at d = 1.6−7.1 kpc from the Sun and at Galactocentric distances 5.5−11.8 kpc, with age in the range 10 Myr to 1.5 Gyr and reddening E(B−V) in the range 0.19−2.56 mag. The core and cluster radii are in the range 0.27−1.88 pc and 2.2−11.27 pc, respectively. Cz 6 and FSR198 are the youngest OCs of this sample, with a population of pre-main sequence (PMS) stars, while FSR 178 is the oldest cluster. |
publishDate |
2009 |
dc.date.issued.fl_str_mv |
2009 |
dc.date.accessioned.fl_str_mv |
2014-08-08T02:07:03Z |
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000827391 |
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http://hdl.handle.net/10183/99263 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Astronomy and astrophysics. Les Ulis. Vol. 508, no. 1 (Dec. 2009), p. 211-220 |
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