The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15
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,...
Guardado en:
| Autores principales: | , , , , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2005
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84401 |
| Aporte de: |
| id |
I19-R120-10915-84401 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| 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 |
| spellingShingle |
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 Carraro, G. Geisler, D. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| topic_facet |
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 |
| 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. |
| format |
Articulo Articulo |
| author |
Carraro, G. Geisler, D. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. |
| author_facet |
Carraro, G. Geisler, D. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. |
| author_sort |
Carraro, G. |
| title |
The intermediate-age open clusters Ruprecht 4, Ruprecht 7 and Pismis 15 |
| 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 |
intermediate-age open clusters ruprecht 4, ruprecht 7 and pismis 15 |
| publishDate |
2005 |
| url |
http://sedici.unlp.edu.ar/handle/10915/84401 |
| work_keys_str_mv |
AT carrarog theintermediateageopenclustersruprecht4ruprecht7andpismis15 AT geislerd theintermediateageopenclustersruprecht4ruprecht7andpismis15 AT baumegustavo theintermediateageopenclustersruprecht4ruprecht7andpismis15 AT vazquezrubenangel theintermediateageopenclustersruprecht4ruprecht7andpismis15 AT moitinhoa theintermediateageopenclustersruprecht4ruprecht7andpismis15 AT carrarog intermediateageopenclustersruprecht4ruprecht7andpismis15 AT geislerd intermediateageopenclustersruprecht4ruprecht7andpismis15 AT baumegustavo intermediateageopenclustersruprecht4ruprecht7andpismis15 AT vazquezrubenangel intermediateageopenclustersruprecht4ruprecht7andpismis15 AT moitinhoa intermediateageopenclustersruprecht4ruprecht7andpismis15 |
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Repositorios |
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1764820488684568578 |