NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc
- Autores
- Carraro, Giovanni; Baume, Gustavo Luis; Villanova, Sandro
- Año de publicación
- 2003
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report on BVI CCD photometry of a field centred in the region of the open cluster NGC 1883, down to V = 21. This cluster has never been studied so far; we provide, for the first time, estimates of its fundamental parameters - namely radial extent, age, distance and reddening. We find that the cluster has a radius of about 2.5 arcmin, and shows signatures of dynamical relaxation. NGC 1883 is located in the anticentre direction, and exhibits a reddening in the range E(B-V) = 0.23-0.35, depending on the metal abundance. It turns out to be of intermediate age (1 Gyr old), and is quite distant for an open cluster. In fact, it is located 4.8 kpc from the Sun, and more than 13 kpc from the Galactic centre. This results makes NGC 1883 one of the most peripheral old open clusters, with important consequences for the trend of the metallicity with distance in the outer Galactic disc.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Astronomía
Hertzsprung–Russell (HR) diagram
open clusters and associations: general
open clusters and associations: individual: NGC 1883 - 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:10915/93899
Ver los metadatos del registro completo
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NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic discCarraro, GiovanniBaume, Gustavo LuisVillanova, SandroAstronomíaHertzsprung–Russell (HR) diagramopen clusters and associations: generalopen clusters and associations: individual: NGC 1883We report on <i>BVI</i> CCD photometry of a field centred in the region of the open cluster NGC 1883, down to V = 21. This cluster has never been studied so far; we provide, for the first time, estimates of its fundamental parameters - namely radial extent, age, distance and reddening. We find that the cluster has a radius of about 2.5 arcmin, and shows signatures of dynamical relaxation. NGC 1883 is located in the anticentre direction, and exhibits a reddening in the range E(B-V) = 0.23-0.35, depending on the metal abundance. It turns out to be of intermediate age (1 Gyr old), and is quite distant for an open cluster. In fact, it is located 4.8 kpc from the Sun, and more than 13 kpc from the Galactic centre. This results makes NGC 1883 one of the most peripheral old open clusters, with important consequences for the trend of the metallicity with distance in the outer Galactic disc.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2003-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf547-551http://sedici.unlp.edu.ar/handle/10915/93899enginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/343/2/547/1041436info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/handle/11336/36975info:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.2003.06693.xinfo:eu-repo/semantics/altIdentifier/hdl/11336/36975info: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:UNLP2025-10-22T17:00:17Zoai:sedici.unlp.edu.ar:10915/93899Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:00:17.486SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
title |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
spellingShingle |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc Carraro, Giovanni Astronomía Hertzsprung–Russell (HR) diagram open clusters and associations: general open clusters and associations: individual: NGC 1883 |
title_short |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
title_full |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
title_fullStr |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
title_full_unstemmed |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
title_sort |
NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc |
dc.creator.none.fl_str_mv |
Carraro, Giovanni Baume, Gustavo Luis Villanova, Sandro |
author |
Carraro, Giovanni |
author_facet |
Carraro, Giovanni Baume, Gustavo Luis Villanova, Sandro |
author_role |
author |
author2 |
Baume, Gustavo Luis Villanova, Sandro |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Astronomía Hertzsprung–Russell (HR) diagram open clusters and associations: general open clusters and associations: individual: NGC 1883 |
topic |
Astronomía Hertzsprung–Russell (HR) diagram open clusters and associations: general open clusters and associations: individual: NGC 1883 |
dc.description.none.fl_txt_mv |
We report on <i>BVI</i> CCD photometry of a field centred in the region of the open cluster NGC 1883, down to V = 21. This cluster has never been studied so far; we provide, for the first time, estimates of its fundamental parameters - namely radial extent, age, distance and reddening. We find that the cluster has a radius of about 2.5 arcmin, and shows signatures of dynamical relaxation. NGC 1883 is located in the anticentre direction, and exhibits a reddening in the range E(B-V) = 0.23-0.35, depending on the metal abundance. It turns out to be of intermediate age (1 Gyr old), and is quite distant for an open cluster. In fact, it is located 4.8 kpc from the Sun, and more than 13 kpc from the Galactic centre. This results makes NGC 1883 one of the most peripheral old open clusters, with important consequences for the trend of the metallicity with distance in the outer Galactic disc. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
description |
We report on <i>BVI</i> CCD photometry of a field centred in the region of the open cluster NGC 1883, down to V = 21. This cluster has never been studied so far; we provide, for the first time, estimates of its fundamental parameters - namely radial extent, age, distance and reddening. We find that the cluster has a radius of about 2.5 arcmin, and shows signatures of dynamical relaxation. NGC 1883 is located in the anticentre direction, and exhibits a reddening in the range E(B-V) = 0.23-0.35, depending on the metal abundance. It turns out to be of intermediate age (1 Gyr old), and is quite distant for an open cluster. In fact, it is located 4.8 kpc from the Sun, and more than 13 kpc from the Galactic centre. This results makes NGC 1883 one of the most peripheral old open clusters, with important consequences for the trend of the metallicity with distance in the outer Galactic disc. |
publishDate |
2003 |
dc.date.none.fl_str_mv |
2003-08 |
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/10915/93899 |
url |
http://sedici.unlp.edu.ar/handle/10915/93899 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/343/2/547/1041436 info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/handle/11336/36975 info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.2003.06693.x info:eu-repo/semantics/altIdentifier/hdl/11336/36975 |
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 547-551 |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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