A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25

Autores
Carraro, G.; Geisler, D.; Moitinho, A.; Baume, Gustavo; Vázquez, Rubén Ángel
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
CCD BVI photometry of the faint open clusters Berkeley 73, Berkeley 75 and Berkeley 25 are presented. The two latter are previously unstudied clusters to our knowledge. While Berkeley 73 is found to be of intermediate-age (about 1.5 Gyr old), Berkeley 75 and Berkeley 25 are old clusters, with ages greater than 3.0 Gyr. We provide also estimates of the clusters size. All these clusters lie far away from the Galactic Center, at R GC ≥ 16 kpc, and quite high on the Galactic plane, at |Z ⊙ | ≥ 1.5 kpc. They are therefore important targets to probe the properties of the structure of the Galaxy in this direction, where the Canis Major over-density has been discovered to be located.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Hertzprung-Russell diagrams
Open clusters and associations: general
C-M diagrams
Berkeley 73
Berkeley 75
Berkeley 25
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:10915/83500
Acceder
id SEDICI_3b48cdd36fb7bfcd46b41084e05acaa7
oai_identifier_str oai:sedici.unlp.edu.ar:10915/83500
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25Carraro, G.Geisler, D.Moitinho, A.Baume, GustavoVázquez, Rubén ÁngelCiencias AstronómicasHertzprung-Russell diagramsOpen clusters and associations: generalC-M diagramsBerkeley 73Berkeley 75Berkeley 25CCD BVI photometry of the faint open clusters Berkeley 73, Berkeley 75 and Berkeley 25 are presented. The two latter are previously unstudied clusters to our knowledge. While Berkeley 73 is found to be of intermediate-age (about 1.5 Gyr old), Berkeley 75 and Berkeley 25 are old clusters, with ages greater than 3.0 Gyr. We provide also estimates of the clusters size. All these clusters lie far away from the Galactic Center, at R GC ≥ 16 kpc, and quite high on the Galactic plane, at |Z ⊙ | ≥ 1.5 kpc. They are therefore important targets to probe the properties of the structure of the Galaxy in this direction, where the Canis Major over-density has been discovered to be located.Facultad de Ciencias Astronómicas y Geofísicas2005-10-14info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf917-924http://sedici.unlp.edu.ar/handle/10915/83500enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20053089info: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:UNLP2025-09-03T10:48:05Zoai:sedici.unlp.edu.ar:10915/83500Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:48:05.745SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
title A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
spellingShingle A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
Carraro, G.
Ciencias Astronómicas
Hertzprung-Russell diagrams
Open clusters and associations: general
C-M diagrams
Berkeley 73
Berkeley 75
Berkeley 25
title_short A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
title_full A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
title_fullStr A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
title_full_unstemmed A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
title_sort A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
dc.creator.none.fl_str_mv Carraro, G.
Geisler, D.
Moitinho, A.
Baume, Gustavo
Vázquez, Rubén Ángel
author Carraro, G.
author_facet Carraro, G.
Geisler, D.
Moitinho, A.
Baume, Gustavo
Vázquez, Rubén Ángel
author_role author
author2 Geisler, D.
Moitinho, A.
Baume, Gustavo
Vázquez, Rubén Ángel
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Hertzprung-Russell diagrams
Open clusters and associations: general
C-M diagrams
Berkeley 73
Berkeley 75
Berkeley 25
topic Ciencias Astronómicas
Hertzprung-Russell diagrams
Open clusters and associations: general
C-M diagrams
Berkeley 73
Berkeley 75
Berkeley 25
dc.description.none.fl_txt_mv CCD BVI photometry of the faint open clusters Berkeley 73, Berkeley 75 and Berkeley 25 are presented. The two latter are previously unstudied clusters to our knowledge. While Berkeley 73 is found to be of intermediate-age (about 1.5 Gyr old), Berkeley 75 and Berkeley 25 are old clusters, with ages greater than 3.0 Gyr. We provide also estimates of the clusters size. All these clusters lie far away from the Galactic Center, at R GC ≥ 16 kpc, and quite high on the Galactic plane, at |Z ⊙ | ≥ 1.5 kpc. They are therefore important targets to probe the properties of the structure of the Galaxy in this direction, where the Canis Major over-density has been discovered to be located.
Facultad de Ciencias Astronómicas y Geofísicas
description CCD BVI photometry of the faint open clusters Berkeley 73, Berkeley 75 and Berkeley 25 are presented. The two latter are previously unstudied clusters to our knowledge. While Berkeley 73 is found to be of intermediate-age (about 1.5 Gyr old), Berkeley 75 and Berkeley 25 are old clusters, with ages greater than 3.0 Gyr. We provide also estimates of the clusters size. All these clusters lie far away from the Galactic Center, at R GC ≥ 16 kpc, and quite high on the Galactic plane, at |Z ⊙ | ≥ 1.5 kpc. They are therefore important targets to probe the properties of the structure of the Galaxy in this direction, where the Canis Major over-density has been discovered to be located.
publishDate 2005
dc.date.none.fl_str_mv 2005-10-14
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/10915/83500
url http://sedici.unlp.edu.ar/handle/10915/83500
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/10.1051/0004-6361:20053089
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
917-924
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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score 13.13397

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