The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262

Autores
Carraro, G.; Baume, Gustavo; Vázquez, Rubén Ángel; Moitinho, A.; Geisler, D.
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the first BVI CCD photometry to V = 22.0 of four fields centred on the region of the southern Galactic star clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262 and of four displaced control fields. These clusters have never been studied before, and we provide for the first time estimates of their fundamental parameters, specifically radial extent, age, distance and reddening. We find that the four clusters are all of intermediate age (around 1 Gyr), close to the Sun and possess lower than solar metal abundance.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
Materia
Ciencias Astronómicas
Open clusters and associations: general
Open clusters and associations: individual: Czernik 32
Open clusters and associations: individual: NGC 2225
Open clusters and associations: individual: Ruprecht 61
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/84361
Acceder
id SEDICI_7138c7af810f0744a040de7dfef9a104
oai_identifier_str oai:sedici.unlp.edu.ar:10915/84361
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262Carraro, G.Baume, GustavoVázquez, Rubén ÁngelMoitinho, A.Geisler, D.Ciencias AstronómicasOpen clusters and associations: generalOpen clusters and associations: individual: Czernik 32Open clusters and associations: individual: NGC 2225Open clusters and associations: individual: Ruprecht 61We present the first <i>BVI</i> CCD photometry to V = 22.0 of four fields centred on the region of the southern Galactic star clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262 and of four displaced control fields. These clusters have never been studied before, and we provide for the first time estimates of their fundamental parameters, specifically radial extent, age, distance and reddening. We find that the four clusters are all of intermediate age (around 1 Gyr), close to the Sun and possess lower than solar metal abundance.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2005info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf649-656http://sedici.unlp.edu.ar/handle/10915/84361enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2005.09340.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:08:07Zoai:sedici.unlp.edu.ar:10915/84361Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:08:07.728SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
title The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
spellingShingle The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
Carraro, G.
Ciencias Astronómicas
Open clusters and associations: general
Open clusters and associations: individual: Czernik 32
Open clusters and associations: individual: NGC 2225
Open clusters and associations: individual: Ruprecht 61
title_short The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
title_full The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
title_fullStr The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
title_full_unstemmed The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
title_sort The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
dc.creator.none.fl_str_mv Carraro, G.
Baume, Gustavo
Vázquez, Rubén Ángel
Moitinho, A.
Geisler, D.
author Carraro, G.
author_facet Carraro, G.
Baume, Gustavo
Vázquez, Rubén Ángel
Moitinho, A.
Geisler, D.
author_role author
author2 Baume, Gustavo
Vázquez, Rubén Ángel
Moitinho, A.
Geisler, D.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Open clusters and associations: general
Open clusters and associations: individual: Czernik 32
Open clusters and associations: individual: NGC 2225
Open clusters and associations: individual: Ruprecht 61
topic Ciencias Astronómicas
Open clusters and associations: general
Open clusters and associations: individual: Czernik 32
Open clusters and associations: individual: NGC 2225
Open clusters and associations: individual: Ruprecht 61
dc.description.none.fl_txt_mv We present the first <i>BVI</i> CCD photometry to V = 22.0 of four fields centred on the region of the southern Galactic star clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262 and of four displaced control fields. These clusters have never been studied before, and we provide for the first time estimates of their fundamental parameters, specifically radial extent, age, distance and reddening. We find that the four clusters are all of intermediate age (around 1 Gyr), close to the Sun and possess lower than solar metal abundance.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
description We present the first <i>BVI</i> CCD photometry to V = 22.0 of four fields centred on the region of the southern Galactic star clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262 and of four displaced control fields. These clusters have never been studied before, and we provide for the first time estimates of their fundamental parameters, specifically radial extent, age, distance and reddening. We find that the four clusters are all of intermediate age (around 1 Gyr), close to the Sun and possess lower than solar metal abundance.
publishDate 2005
dc.date.none.fl_str_mv 2005
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/84361
url http://sedici.unlp.edu.ar/handle/10915/84361
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0035-8711
info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2005.09340.x
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
649-656
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.22299

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