The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262
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 fi...
| Autores principales: | , , , , |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2005
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84361 |
| Aporte de: |
| id |
I19-R120-10915-84361 |
|---|---|
| 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: Czernik 32 Open clusters and associations: individual: NGC 2225 Open clusters and associations: individual: Ruprecht 61 |
| spellingShingle |
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 Carraro, G. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. Geisler, D. The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262 |
| topic_facet |
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 |
| 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. |
| format |
Articulo Articulo |
| author |
Carraro, G. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. Geisler, D. |
| author_facet |
Carraro, G. Baume, Gustavo Vázquez, Rubén Ángel Moitinho, A. Geisler, D. |
| author_sort |
Carraro, G. |
| title |
The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and 2262 |
| 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 |
intermediate-age open clusters ruprecht 61, czernik 32, ngc 2225 and 2262 |
| publishDate |
2005 |
| url |
http://sedici.unlp.edu.ar/handle/10915/84361 |
| work_keys_str_mv |
AT carrarog theintermediateageopenclustersruprecht61czernik32ngc2225and2262 AT baumegustavo theintermediateageopenclustersruprecht61czernik32ngc2225and2262 AT vazquezrubenangel theintermediateageopenclustersruprecht61czernik32ngc2225and2262 AT moitinhoa theintermediateageopenclustersruprecht61czernik32ngc2225and2262 AT geislerd theintermediateageopenclustersruprecht61czernik32ngc2225and2262 AT carrarog intermediateageopenclustersruprecht61czernik32ngc2225and2262 AT baumegustavo intermediateageopenclustersruprecht61czernik32ngc2225and2262 AT vazquezrubenangel intermediateageopenclustersruprecht61czernik32ngc2225and2262 AT moitinhoa intermediateageopenclustersruprecht61czernik32ngc2225and2262 AT geislerd intermediateageopenclustersruprecht61czernik32ngc2225and2262 |
| bdutipo_str |
Repositorios |
| _version_ |
1764820488638431235 |