Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447

Autores
Claria Olmedo, Juan Jose; Piatti, Andres Eduardo; Lapasset Gomar, Emilio; Parisi, Maria Celeste
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Photoelectric photometry in the UBV, DDO and Washington systems is presented for 14 late-type giant candidates of the southern open cluster NGC 2447. By applying two independent photometric criteria, nine stars are found to have a high probability of being cluster giants. The photometric membership results are in good agreement with those derived from published Coravel radial velocities. The mean interstellar reddening EB-V = 0.05±0.04 has been derived from the confirmed cluster giants. NGC 2447 has a mean ultraviolet excess <δ (U-B)> = 0.01±0.02 (σ n) with respect to solar composition K giants, and a mean cyanogen anomaly <Δ CN> = 0.01±0.02 (σ n), both implying a small metal deficiency ([Fe/H] ≃ -0.1). Five independent Washington abundance indices yield a mean cluster metallicity of [Fe/H] = -0.09±0.06, in agreement with the two previous estimates. Therefore, NGC 2447 is found to be slightly metal-poor.
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Lapasset Gomar, Emilio. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Parisi, Maria Celeste. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
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:11336/81808

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spelling Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447Claria Olmedo, Juan JosePiatti, Andres EduardoLapasset Gomar, EmilioParisi, Maria Celestehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Photoelectric photometry in the UBV, DDO and Washington systems is presented for 14 late-type giant candidates of the southern open cluster NGC 2447. By applying two independent photometric criteria, nine stars are found to have a high probability of being cluster giants. The photometric membership results are in good agreement with those derived from published Coravel radial velocities. The mean interstellar reddening E<sub>B-V</sub> = 0.05±0.04 has been derived from the confirmed cluster giants. NGC 2447 has a mean ultraviolet excess <δ (U-B)> = 0.01±0.02 (σ <sub>n</sub>) with respect to solar composition K giants, and a mean cyanogen anomaly <Δ CN> = 0.01±0.02 (σ <sub>n</sub>), both implying a small metal deficiency ([Fe/H] ≃ -0.1). Five independent Washington abundance indices yield a mean cluster metallicity of [Fe/H] = -0.09±0.06, in agreement with the two previous estimates. Therefore, NGC 2447 is found to be slightly metal-poor.Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Lapasset Gomar, Emilio. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Parisi, Maria Celeste. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaInst Theoretical Physics Astronomy2005-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/81808Claria Olmedo, Juan Jose; Piatti, Andres Eduardo; Lapasset Gomar, Emilio; Parisi, Maria Celeste; Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447; Inst Theoretical Physics Astronomy; Baltic Astronomy; 14; 12-2005; 301-3111392-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-02-26T10:08:08Zoai:ri.conicet.gov.ar:11336/81808instacron: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:34982026-02-26 10:08:08.983CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
title Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
spellingShingle Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
Claria Olmedo, Juan Jose
title_short Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
title_full Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
title_fullStr Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
title_full_unstemmed Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
title_sort Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447
dc.creator.none.fl_str_mv Claria Olmedo, Juan Jose
Piatti, Andres Eduardo
Lapasset Gomar, Emilio
Parisi, Maria Celeste
author Claria Olmedo, Juan Jose
author_facet Claria Olmedo, Juan Jose
Piatti, Andres Eduardo
Lapasset Gomar, Emilio
Parisi, Maria Celeste
author_role author
author2 Piatti, Andres Eduardo
Lapasset Gomar, Emilio
Parisi, Maria Celeste
author2_role author
author
author
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Photoelectric photometry in the UBV, DDO and Washington systems is presented for 14 late-type giant candidates of the southern open cluster NGC 2447. By applying two independent photometric criteria, nine stars are found to have a high probability of being cluster giants. The photometric membership results are in good agreement with those derived from published Coravel radial velocities. The mean interstellar reddening E<sub>B-V</sub> = 0.05±0.04 has been derived from the confirmed cluster giants. NGC 2447 has a mean ultraviolet excess <δ (U-B)> = 0.01±0.02 (σ <sub>n</sub>) with respect to solar composition K giants, and a mean cyanogen anomaly <Δ CN> = 0.01±0.02 (σ <sub>n</sub>), both implying a small metal deficiency ([Fe/H] ≃ -0.1). Five independent Washington abundance indices yield a mean cluster metallicity of [Fe/H] = -0.09±0.06, in agreement with the two previous estimates. Therefore, NGC 2447 is found to be slightly metal-poor.
Fil: Claria Olmedo, Juan Jose. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Lapasset Gomar, Emilio. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Parisi, Maria Celeste. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
description Photoelectric photometry in the UBV, DDO and Washington systems is presented for 14 late-type giant candidates of the southern open cluster NGC 2447. By applying two independent photometric criteria, nine stars are found to have a high probability of being cluster giants. The photometric membership results are in good agreement with those derived from published Coravel radial velocities. The mean interstellar reddening E<sub>B-V</sub> = 0.05±0.04 has been derived from the confirmed cluster giants. NGC 2447 has a mean ultraviolet excess <δ (U-B)> = 0.01±0.02 (σ <sub>n</sub>) with respect to solar composition K giants, and a mean cyanogen anomaly <Δ CN> = 0.01±0.02 (σ <sub>n</sub>), both implying a small metal deficiency ([Fe/H] ≃ -0.1). Five independent Washington abundance indices yield a mean cluster metallicity of [Fe/H] = -0.09±0.06, in agreement with the two previous estimates. Therefore, NGC 2447 is found to be slightly metal-poor.
publishDate 2005
dc.date.none.fl_str_mv 2005-12
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/11336/81808
Claria Olmedo, Juan Jose; Piatti, Andres Eduardo; Lapasset Gomar, Emilio; Parisi, Maria Celeste; Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447; Inst Theoretical Physics Astronomy; Baltic Astronomy; 14; 12-2005; 301-311
1392-0049
CONICET Digital
CONICET
url http://hdl.handle.net/11336/81808
identifier_str_mv Claria Olmedo, Juan Jose; Piatti, Andres Eduardo; Lapasset Gomar, Emilio; Parisi, Maria Celeste; Multicolor Photometry of Red Giant Candidates in the Southern Open Cluster NGC 2447; Inst Theoretical Physics Astronomy; Baltic Astronomy; 14; 12-2005; 301-311
1392-0049
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
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
dc.publisher.none.fl_str_mv Inst Theoretical Physics Astronomy
publisher.none.fl_str_mv Inst Theoretical Physics Astronomy
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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