A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates

Aims. Based on stellar positions and proper motions, we aim to re-analyse the region of the controversial open cluster Collinder 132. Methods. We have developed a model which analyses the proper motion distribution and the stellar density to find moving groups. The astrometric data were obtained fro...

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Autores principales: Orellana, Rosa Beatriz, De Biasi, María Silvina, Bustos Fierro, I. H., Calderón, J. H.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2010
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/82529
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id I19-R120-10915-82529
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Astrometry
Open clusters and associations: general
Open clusters and associations: individual: Cr132
spellingShingle Ciencias Astronómicas
Astrometry
Open clusters and associations: general
Open clusters and associations: individual: Cr132
Orellana, Rosa Beatriz
De Biasi, María Silvina
Bustos Fierro, I. H.
Calderón, J. H.
A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates
topic_facet Ciencias Astronómicas
Astrometry
Open clusters and associations: general
Open clusters and associations: individual: Cr132
description Aims. Based on stellar positions and proper motions, we aim to re-analyse the region of the controversial open cluster Collinder 132. Methods. We have developed a model which analyses the proper motion distribution and the stellar density to find moving groups. The astrometric data were obtained from four Carte du Ciel (CdC) and one Astrogaphic Catalogue (AC) plates of the Córdoba Astronomical Observatory collection (Argentina). Results. We detected an open cluster from the field stars and calculated the mean proper motion and the membership probabilities of the region's stars. We report new coordinates of its centre αc = 108\fdg347, δc = -31\fdg011, the components of mean proper motion μ αcosδ = -2.62±0.44 mas/yr, μδ = 4.79±0.88 mas/yr. Thirteen stars are astrometric members giving a value of 20' for the cluster angular diameter. Six stars fulfil the astrometric and photometric criteria for being cluster members and locate the cluster at 360 pc from the Sun. We propose a simple model for the analysis of the proper motion distribution of an association. We report the components of the association mean proper motion μαcosδ = -1.38±0.14 mas/yr, μδ = 2.26±0.16 mas/yr. We found 149 astrometric members, 11 of which have reliable photometric data that locate them betweeen 417 and 660 pc from the Sun.
format Articulo
Articulo
author Orellana, Rosa Beatriz
De Biasi, María Silvina
Bustos Fierro, I. H.
Calderón, J. H.
author_facet Orellana, Rosa Beatriz
De Biasi, María Silvina
Bustos Fierro, I. H.
Calderón, J. H.
author_sort Orellana, Rosa Beatriz
title A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates
title_short A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates
title_full A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates
title_fullStr A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates
title_full_unstemmed A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates
title_sort revisit to the region of collinder 132 using carte du ciel and astrographic catalogue plates
publishDate 2010
url http://sedici.unlp.edu.ar/handle/10915/82529
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