On the nature of five open cluster candidates projected close to the Galactic centre

We present CCD BV I observations obtained for 1759 stars in 4′×4′ regions around the unstudied southern stellar aggregates Ruprecht 103, 124, 129, 146 and 166, which are described as open clusters in several catalogues. Our analysis shows that none of these stellar groups are genuine open clusters s...

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Autores principales: Piatti, A.E., Clariá, J.J.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v379_n2_p453_Piatti
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spelling todo:paper_00046361_v379_n2_p453_Piatti2023-10-03T13:59:58Z On the nature of five open cluster candidates projected close to the Galactic centre Piatti, A.E. Clariá, J.J. Open clusters and associations: general Open clusters and associations: individual: Ruprecht 103, 124, 129, 146, and 166 We present CCD BV I observations obtained for 1759 stars in 4′×4′ regions around the unstudied southern stellar aggregates Ruprecht 103, 124, 129, 146 and 166, which are described as open clusters in several catalogues. Our analysis shows that none of these stellar groups are genuine open clusters since no clear main sequences or other meaningful features can be seen in their colour-magnitude diagrams. Star counts carried out within and outside the cluster candidate fields not only support these results but also show that the studied objects do not appear to be candidate late stages of star cluster dynamical evolution. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v379_n2_p453_Piatti
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Open clusters and associations: general
Open clusters and associations: individual: Ruprecht 103, 124, 129, 146, and 166
spellingShingle Open clusters and associations: general
Open clusters and associations: individual: Ruprecht 103, 124, 129, 146, and 166
Piatti, A.E.
Clariá, J.J.
On the nature of five open cluster candidates projected close to the Galactic centre
topic_facet Open clusters and associations: general
Open clusters and associations: individual: Ruprecht 103, 124, 129, 146, and 166
description We present CCD BV I observations obtained for 1759 stars in 4′×4′ regions around the unstudied southern stellar aggregates Ruprecht 103, 124, 129, 146 and 166, which are described as open clusters in several catalogues. Our analysis shows that none of these stellar groups are genuine open clusters since no clear main sequences or other meaningful features can be seen in their colour-magnitude diagrams. Star counts carried out within and outside the cluster candidate fields not only support these results but also show that the studied objects do not appear to be candidate late stages of star cluster dynamical evolution.
format JOUR
author Piatti, A.E.
Clariá, J.J.
author_facet Piatti, A.E.
Clariá, J.J.
author_sort Piatti, A.E.
title On the nature of five open cluster candidates projected close to the Galactic centre
title_short On the nature of five open cluster candidates projected close to the Galactic centre
title_full On the nature of five open cluster candidates projected close to the Galactic centre
title_fullStr On the nature of five open cluster candidates projected close to the Galactic centre
title_full_unstemmed On the nature of five open cluster candidates projected close to the Galactic centre
title_sort on the nature of five open cluster candidates projected close to the galactic centre
url http://hdl.handle.net/20.500.12110/paper_00046361_v379_n2_p453_Piatti
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