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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84361
Ver los metadatos del registro completo
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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:UNLP2025-09-29T11:16:14Zoai: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:13292025-09-29 11:16:15.256SEDICI (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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13.070432 |