Hogg 12 and NGC 3590: A new open cluster binary system candidate

Autores
Piatti, Andres Eduardo; Claria Olmedo, Juan Jose; Ahumada, Andrea Veronica
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We have obtained CCD UBVI(KC) photometry down to V = 22 for the open clusters Hogg 12 and NGC 3590 and their surrounding fields. We confirm the physical reality of Hogg 12 like a genuine open cluster from photometric, morphologican and space density criteria; NGC 3590 served as a control cluster. The extracted-cleaned photometry of Hogg 12 reveals that the cluster is of solar metal content, affected by a E(B-V) color excess of 0.40 mag, and placed at a distance from the Sun of d = 2.0 kpc, if a Sun´s distance from the center of the Galaxy of 8.5 kpc is assumed. Hogg 12 appears to be as old as NGC 3590 (t = 30 Myr). Both clusters are surprisingly small objects with radii of approximately 1 pc and scarsely separated by 3.6 pc, which, besides to their similar ages, reddenings and metallicities, becomes them in a new candidate open cluster binary system. Out of approximately 180 open cluster binary systems estimated to exist in the Galaxy, they are one of the two closest pairs between 27 actaully known.
Fil: Piatti, Andres Eduardo. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Ahumada, Andrea Veronica. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Materia
GALAXY
TECHNIQUES: PHOTOMETRY
STAR CLUSTERS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/94131
Acceder
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Hogg 12 and NGC 3590: A new open cluster binary system candidatePiatti, Andres EduardoClaria Olmedo, Juan JoseAhumada, Andrea VeronicaGALAXYTECHNIQUES: PHOTOMETRYSTAR CLUSTERShttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We have obtained CCD UBVI(KC) photometry down to V = 22 for the open clusters Hogg 12 and NGC 3590 and their surrounding fields. We confirm the physical reality of Hogg 12 like a genuine open cluster from photometric, morphologican and space density criteria; NGC 3590 served as a control cluster. The extracted-cleaned photometry of Hogg 12 reveals that the cluster is of solar metal content, affected by a E(B-V) color excess of 0.40 mag, and placed at a distance from the Sun of d = 2.0 kpc, if a Sun´s distance from the center of the Galaxy of 8.5 kpc is assumed. Hogg 12 appears to be as old as NGC 3590 (t = 30 Myr). Both clusters are surprisingly small objects with radii of approximately 1 pc and scarsely separated by 3.6 pc, which, besides to their similar ages, reddenings and metallicities, becomes them in a new candidate open cluster binary system. Out of approximately 180 open cluster binary systems estimated to exist in the Galaxy, they are one of the two closest pairs between 27 actaully known.Fil: Piatti, Andres Eduardo. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaFil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaFil: Ahumada, Andrea Veronica. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; ArgentinaUniversity of Chicago Press2010-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/94131Piatti, Andres Eduardo; Claria Olmedo, Juan Jose; Ahumada, Andrea Veronica; Hogg 12 and NGC 3590: A new open cluster binary system candidate; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 122; 891; 5-2010; 516-5230004-62801538-3873CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/652501info:eu-repo/semantics/altIdentifier/doi/10.1086/652501info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:21:28Zoai:ri.conicet.gov.ar:11336/94131instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:21:28.725CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Hogg 12 and NGC 3590: A new open cluster binary system candidate
title Hogg 12 and NGC 3590: A new open cluster binary system candidate
spellingShingle Hogg 12 and NGC 3590: A new open cluster binary system candidate
Piatti, Andres Eduardo
GALAXY
TECHNIQUES: PHOTOMETRY
STAR CLUSTERS
title_short Hogg 12 and NGC 3590: A new open cluster binary system candidate
title_full Hogg 12 and NGC 3590: A new open cluster binary system candidate
title_fullStr Hogg 12 and NGC 3590: A new open cluster binary system candidate
title_full_unstemmed Hogg 12 and NGC 3590: A new open cluster binary system candidate
title_sort Hogg 12 and NGC 3590: A new open cluster binary system candidate
dc.creator.none.fl_str_mv Piatti, Andres Eduardo
Claria Olmedo, Juan Jose
Ahumada, Andrea Veronica
author Piatti, Andres Eduardo
author_facet Piatti, Andres Eduardo
Claria Olmedo, Juan Jose
Ahumada, Andrea Veronica
author_role author
author2 Claria Olmedo, Juan Jose
Ahumada, Andrea Veronica
author2_role author
author
dc.subject.none.fl_str_mv GALAXY
TECHNIQUES: PHOTOMETRY
STAR CLUSTERS
topic GALAXY
TECHNIQUES: PHOTOMETRY
STAR CLUSTERS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We have obtained CCD UBVI(KC) photometry down to V = 22 for the open clusters Hogg 12 and NGC 3590 and their surrounding fields. We confirm the physical reality of Hogg 12 like a genuine open cluster from photometric, morphologican and space density criteria; NGC 3590 served as a control cluster. The extracted-cleaned photometry of Hogg 12 reveals that the cluster is of solar metal content, affected by a E(B-V) color excess of 0.40 mag, and placed at a distance from the Sun of d = 2.0 kpc, if a Sun´s distance from the center of the Galaxy of 8.5 kpc is assumed. Hogg 12 appears to be as old as NGC 3590 (t = 30 Myr). Both clusters are surprisingly small objects with radii of approximately 1 pc and scarsely separated by 3.6 pc, which, besides to their similar ages, reddenings and metallicities, becomes them in a new candidate open cluster binary system. Out of approximately 180 open cluster binary systems estimated to exist in the Galaxy, they are one of the two closest pairs between 27 actaully known.
Fil: Piatti, Andres Eduardo. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
Fil: Ahumada, Andrea Veronica. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Departamento de Astrofísica Estelar; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina
description We have obtained CCD UBVI(KC) photometry down to V = 22 for the open clusters Hogg 12 and NGC 3590 and their surrounding fields. We confirm the physical reality of Hogg 12 like a genuine open cluster from photometric, morphologican and space density criteria; NGC 3590 served as a control cluster. The extracted-cleaned photometry of Hogg 12 reveals that the cluster is of solar metal content, affected by a E(B-V) color excess of 0.40 mag, and placed at a distance from the Sun of d = 2.0 kpc, if a Sun´s distance from the center of the Galaxy of 8.5 kpc is assumed. Hogg 12 appears to be as old as NGC 3590 (t = 30 Myr). Both clusters are surprisingly small objects with radii of approximately 1 pc and scarsely separated by 3.6 pc, which, besides to their similar ages, reddenings and metallicities, becomes them in a new candidate open cluster binary system. Out of approximately 180 open cluster binary systems estimated to exist in the Galaxy, they are one of the two closest pairs between 27 actaully known.
publishDate 2010
dc.date.none.fl_str_mv 2010-05
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/94131
Piatti, Andres Eduardo; Claria Olmedo, Juan Jose; Ahumada, Andrea Veronica; Hogg 12 and NGC 3590: A new open cluster binary system candidate; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 122; 891; 5-2010; 516-523
0004-6280
1538-3873
CONICET Digital
CONICET
url http://hdl.handle.net/11336/94131
identifier_str_mv Piatti, Andres Eduardo; Claria Olmedo, Juan Jose; Ahumada, Andrea Veronica; Hogg 12 and NGC 3590: A new open cluster binary system candidate; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 122; 891; 5-2010; 516-523
0004-6280
1538-3873
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/652501
info:eu-repo/semantics/altIdentifier/doi/10.1086/652501
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv University of Chicago Press
publisher.none.fl_str_mv University of Chicago Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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