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
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/83270
Acceder
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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:UNLP2025-10-15T11:07:42Zoai: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:13292025-10-15 11:07:42.553SEDICI (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
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