Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635
- Autores
- Moitinho, A.; Carraro, G.; Baume, Gustavo; Vázquez, Rubén Ángel
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Galaxy: open clusters and associations: Individual: NGC 2425, NGC 2635 - 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:10915/83270
Ver los metadatos del registro completo
id |
SEDICI_daceaaca7fa627c554dd778a1ab71086 |
---|---|
oai_identifier_str |
oai:sedici.unlp.edu.ar:10915/83270 |
network_acronym_str |
SEDICI |
repository_id_str |
1329 |
network_name_str |
SEDICI (UNLP) |
spelling |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635Moitinho, A.Carraro, G.Baume, GustavoVázquez, Rubén ÁngelCiencias AstronómicasGalaxy: open clusters and associations: Individual: NGC 2425, NGC 2635We 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.Facultad de Ciencias Astronómicas y Geofísicas2006info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf493-501http://sedici.unlp.edu.ar/handle/10915/83270enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20053254info: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:UNLP2025-09-29T11:15:46Zoai:sedici.unlp.edu.ar:10915/83270Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:46.852SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
title |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
spellingShingle |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 Moitinho, A. Ciencias Astronómicas Galaxy: open clusters and associations: Individual: NGC 2425, NGC 2635 |
title_short |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
title_full |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
title_fullStr |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
title_full_unstemmed |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
title_sort |
Open clusters in the third Galactic Quadrant : II. The intermediate age open clusters NGC 2425 and NGC 2635 |
dc.creator.none.fl_str_mv |
Moitinho, A. Carraro, G. Baume, Gustavo Vázquez, Rubén Ángel |
author |
Moitinho, A. |
author_facet |
Moitinho, A. Carraro, G. Baume, Gustavo Vázquez, Rubén Ángel |
author_role |
author |
author2 |
Carraro, G. Baume, Gustavo Vázquez, Rubén Ángel |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxy: open clusters and associations: Individual: NGC 2425, NGC 2635 |
topic |
Ciencias Astronómicas Galaxy: open clusters and associations: Individual: NGC 2425, NGC 2635 |
dc.description.none.fl_txt_mv |
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. Facultad de Ciencias Astronómicas y Geofísicas |
description |
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. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006 |
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/10915/83270 |
url |
http://sedici.unlp.edu.ar/handle/10915/83270 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20053254 |
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 493-501 |
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 |
_version_ |
1844616030151770112 |
score |
13.070432 |