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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/94131
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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 Técnicas2025-09-29T09:52:02Zoai: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:34982025-09-29 09:52:03.194CONICET 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 |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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