The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15
- Autores
- Carraro, G.; Geisler, D.; Baume, Gustavo; Vázquez, Rubén Ángel; Moitinho, A.
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report on BVI CCD photometry to V = 22.0 for three fields centred on the region of the Galactic Star clusters Ruprecht 4, Ruprecht 7 and Pismis 15 and on three displaced control fields. Ruprecht 4 and Pismis 15 have never been studied before, and we provide, for the first time, estimates of their fundamental parameters, namely, radial extent, age, distance and reddening. Ruprecht 7 (Berkeley 33), however, was studied by Mazur, Kaluzny & Krzeminski. We find that the three clusters are all of intermediate age (0.8-1. 3 Gyr), and with a metallicity close to or lower than solar.
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: Pismis 15
Open clusters and associations: individual: Ruprecht 4
Open clusters and associations: individual: Ruprecht 7 - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84401
Ver los metadatos del registro completo
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The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15Carraro, G.Geisler, D.Baume, GustavoVázquez, Rubén ÁngelMoitinho, A.Ciencias AstronómicasOpen clusters and associations: generalOpen clusters and associations: individual: Pismis 15Open clusters and associations: individual: Ruprecht 4Open clusters and associations: individual: Ruprecht 7We report on <i>BVI</i> CCD photometry to V = 22.0 for three fields centred on the region of the Galactic Star clusters Ruprecht 4, Ruprecht 7 and Pismis 15 and on three displaced control fields. Ruprecht 4 and Pismis 15 have never been studied before, and we provide, for the first time, estimates of their fundamental parameters, namely, radial extent, age, distance and reddening. Ruprecht 7 (Berkeley 33), however, was studied by Mazur, Kaluzny & Krzeminski. We find that the three clusters are all of intermediate age (0.8-1. 3 Gyr), and with a metallicity close to or lower than solar.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/pdf655-661http://sedici.unlp.edu.ar/handle/10915/84401enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2005.09054.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:UNLP2025-11-12T10:40:29Zoai:sedici.unlp.edu.ar:10915/84401Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-11-12 10:40:29.343SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| title |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| spellingShingle |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 Carraro, G. Ciencias Astronómicas Open clusters and associations: general Open clusters and associations: individual: Pismis 15 Open clusters and associations: individual: Ruprecht 4 Open clusters and associations: individual: Ruprecht 7 |
| title_short |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| title_full |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| title_fullStr |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| title_full_unstemmed |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| title_sort |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| dc.creator.none.fl_str_mv |
Carraro, G. Geisler, D. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. |
| author |
Carraro, G. |
| author_facet |
Carraro, G. Geisler, D. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. |
| author_role |
author |
| author2 |
Geisler, D. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. |
| author2_role |
author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Open clusters and associations: general Open clusters and associations: individual: Pismis 15 Open clusters and associations: individual: Ruprecht 4 Open clusters and associations: individual: Ruprecht 7 |
| topic |
Ciencias Astronómicas Open clusters and associations: general Open clusters and associations: individual: Pismis 15 Open clusters and associations: individual: Ruprecht 4 Open clusters and associations: individual: Ruprecht 7 |
| dc.description.none.fl_txt_mv |
We report on <i>BVI</i> CCD photometry to V = 22.0 for three fields centred on the region of the Galactic Star clusters Ruprecht 4, Ruprecht 7 and Pismis 15 and on three displaced control fields. Ruprecht 4 and Pismis 15 have never been studied before, and we provide, for the first time, estimates of their fundamental parameters, namely, radial extent, age, distance and reddening. Ruprecht 7 (Berkeley 33), however, was studied by Mazur, Kaluzny & Krzeminski. We find that the three clusters are all of intermediate age (0.8-1. 3 Gyr), and with a metallicity close to or lower than solar. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
| description |
We report on <i>BVI</i> CCD photometry to V = 22.0 for three fields centred on the region of the Galactic Star clusters Ruprecht 4, Ruprecht 7 and Pismis 15 and on three displaced control fields. Ruprecht 4 and Pismis 15 have never been studied before, and we provide, for the first time, estimates of their fundamental parameters, namely, radial extent, age, distance and reddening. Ruprecht 7 (Berkeley 33), however, was studied by Mazur, Kaluzny & Krzeminski. We find that the three clusters are all of intermediate age (0.8-1. 3 Gyr), and with a metallicity close to or lower than solar. |
| publishDate |
2005 |
| dc.date.none.fl_str_mv |
2005 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/84401 |
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http://sedici.unlp.edu.ar/handle/10915/84401 |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2005.09054.x |
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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) |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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