NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc
- Autores
- Carraro, Giovanni; Baume, Gustavo Luis; Villanova, S.
- 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.
Fil: Carraro, Giovanni. Università di Padova; Italia
Fil: Baume, Gustavo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Università di Padova; Italia
Fil: Villanova, S.. Università di Padova; Italia - Materia
-
Hertzsprung, Russell (HR) diagram
Open clusters
NGC 1883 (galaxia)
Associations
Photometry - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/36975
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, S.Hertzsprung, Russell (HR) diagramOpen clustersNGC 1883 (galaxia)AssociationsPhotometryhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We 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.Fil: Carraro, Giovanni. Università di Padova; ItaliaFil: Baume, Gustavo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Università di Padova; ItaliaFil: Villanova, S.. Università di Padova; ItaliaWiley Blackwell Publishing, Inc2003-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/36975Carraro, Giovanni; Baume, Gustavo Luis; Villanova, S.; NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 343; 8-2003; 547-5510035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/343/2/547/1041436info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.2003.06693.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:05:56Zoai:ri.conicet.gov.ar:11336/36975instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:05:56.27CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| 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 Hertzsprung, Russell (HR) diagram Open clusters NGC 1883 (galaxia) Associations Photometry |
| 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, S. |
| author |
Carraro, Giovanni |
| author_facet |
Carraro, Giovanni Baume, Gustavo Luis Villanova, S. |
| author_role |
author |
| author2 |
Baume, Gustavo Luis Villanova, S. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Hertzsprung, Russell (HR) diagram Open clusters NGC 1883 (galaxia) Associations Photometry |
| topic |
Hertzsprung, Russell (HR) diagram Open clusters NGC 1883 (galaxia) Associations Photometry |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
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. Fil: Carraro, Giovanni. Università di Padova; Italia Fil: Baume, Gustavo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. Università di Padova; Italia Fil: Villanova, S.. Università di Padova; Italia |
| description |
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. |
| publishDate |
2003 |
| dc.date.none.fl_str_mv |
2003-08 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/36975 Carraro, Giovanni; Baume, Gustavo Luis; Villanova, S.; NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 343; 8-2003; 547-551 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/36975 |
| identifier_str_mv |
Carraro, Giovanni; Baume, Gustavo Luis; Villanova, S.; NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 343; 8-2003; 547-551 0035-8711 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/343/2/547/1041436 info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.2003.06693.x |
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Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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