The open cluster NGC 5662 and its neighboring cepheid V Centauri

Based on new photometric and kinematical data the structure and stellar composition of the open cluster NGC 5662 is examined. The presence of differential reddening across the cluster field is detected and the cluster stability examined. The luminosity function, distance, age, and chemical compositi...

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Detalles Bibliográficos
Autores principales: Clariá, J. J., Lapasset, Emilio, Bosio, Maria Alejandra
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1990
Materias:
Astronomía
Galaxia
ngc 5662
v cen
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/142640
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-142640
record_format dspace
spelling I19-R120-10915-1426402024-09-17T18:39:18Z http://sedici.unlp.edu.ar/handle/10915/142640 The open cluster NGC 5662 and its neighboring cepheid V Centauri Clariá, J. J. Lapasset, Emilio Bosio, Maria Alejandra 1990 2022-09-23T12:54:06Z es Astronomía Galaxia ngc 5662 v cen Based on new photometric and kinematical data the structure and stellar composition of the open cluster NGC 5662 is examined. The presence of differential reddening across the cluster field is detected and the cluster stability examined. The luminosity function, distance, age, and chemical composition of NGC 5662 are determined from photometric and spectroscopic data. The new astrophysical parameters derived support the conclusion that the Cepheid V Cen (P=5.5 days) is very likely a cluster member. The UBV, DDO, CMT1T2 observations and the detailed results obtained in this work have been recently published by Clariá et al. (1991). Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
ngc 5662
v cen
spellingShingle Astronomía
Galaxia
ngc 5662
v cen
Clariá, J. J.
Lapasset, Emilio
Bosio, Maria Alejandra
The open cluster NGC 5662 and its neighboring cepheid V Centauri
topic_facet Astronomía
Galaxia
ngc 5662
v cen
description Based on new photometric and kinematical data the structure and stellar composition of the open cluster NGC 5662 is examined. The presence of differential reddening across the cluster field is detected and the cluster stability examined. The luminosity function, distance, age, and chemical composition of NGC 5662 are determined from photometric and spectroscopic data. The new astrophysical parameters derived support the conclusion that the Cepheid V Cen (P=5.5 days) is very likely a cluster member. The UBV, DDO, CMT1T2 observations and the detailed results obtained in this work have been recently published by Clariá et al. (1991).
format Articulo
Comunicacion
author Clariá, J. J.
Lapasset, Emilio
Bosio, Maria Alejandra
author_facet Clariá, J. J.
Lapasset, Emilio
Bosio, Maria Alejandra
author_sort Clariá, J. J.
title The open cluster NGC 5662 and its neighboring cepheid V Centauri
title_short The open cluster NGC 5662 and its neighboring cepheid V Centauri
title_full The open cluster NGC 5662 and its neighboring cepheid V Centauri
title_fullStr The open cluster NGC 5662 and its neighboring cepheid V Centauri
title_full_unstemmed The open cluster NGC 5662 and its neighboring cepheid V Centauri
title_sort open cluster ngc 5662 and its neighboring cepheid v centauri
publishDate 1990
url http://sedici.unlp.edu.ar/handle/10915/142640
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AT clariajj openclusterngc5662anditsneighboringcepheidvcentauri
AT lapassetemilio openclusterngc5662anditsneighboringcepheidvcentauri
AT bosiomariaalejandra openclusterngc5662anditsneighboringcepheidvcentauri
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