Open clusters in the third galactic quadrant - II. The intermediate age open clusters NGC 2425 and NGC 2635
| Author | dc.contributor.author | Moitinho, A. | |
| Author | dc.contributor.author | Carraro, Giovanni | es_CL |
| Author | dc.contributor.author | Baume, Gustavo | es_CL |
| Author | dc.contributor.author | Vázquez, Rúben A. | es_CL |
| Admission date | dc.date.accessioned | 2009-05-25T12:56:51Z | |
| Available date | dc.date.available | 2009-05-25T12:56:51Z | |
| Publication date | dc.date.issued | 2006-01 | |
| Cita de ítem | dc.identifier.citation | ASTRONOMY & ASTROPHYSICS Volume: 445 Issue: 2 Pages: 493-501 Published: JAN 2006 | en |
| Identifier | dc.identifier.issn | 0004-6361 | |
| Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/124933 | |
| Abstract | dc.description.abstract | We analyse CCD broad band (UBV(RI)(C)) photometric data obtained in the fields of the poorly studied open clusters NGC 2425 and NGC 2635. Both clusters are found to be of intermediate age thus increasing the population of open clusters known to be of the age of, or older than, the Hyades. More explicitly, we find that NGC 2425 is a 2.2 Gyr old cluster, probably of solar metallicity, located at 3.5 kpc from the Sun. NGC 2635 is a Hyades age (600 Myr) cluster located at a distance of 4.0 kpc from the Sun. Its Colour Magnitude Diagram reveals that it is extremely metal poor for its age and position, thus making it a very interesting object in the context of Galactic Disk chemical evolution models. | en |
| Lenguage | dc.language.iso | en | en |
| Publisher | dc.publisher | EDP SCIENCES | en |
| Keywords | dc.subject | OLD OPEN CLUSTERS | en |
| Título | dc.title | Open clusters in the third galactic quadrant - II. The intermediate age open clusters NGC 2425 and NGC 2635 | en |
| Document type | dc.type | Artículo de revista |
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