Open clusters as tracers of the evolution of the Galaxy

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dc.creatorKaluzny, Janusz
dc.creatorKrzeminski, Wojtek
dc.creatorMazur, Beata
dc.date1994-11-18
dc.date.accessioned2026-07-07T02:19:35Z
dc.date.available2026-07-07T02:19:35Z
dc.descriptionDeep color-magnitude diagrams are presented for poorly known open clusters Cr 261, Be 18, Be 54, Tr 5 and BH176. All clusters are old objects with age\geq 4 Gyr. BH176 is either old open cluster or young globular cluster. Extremely red giants with V-I>3 were identified in the central parts of Cr 261, Be 54 and BH176. These three objects are candidates for very metal-rich clusters.
dc.description2 pages, uuencoded compressed postscript
dc.identifierhttps://arxiv.org/abs/astro-ph/9411077
dc.identifierhttp://arxiv.org/abs/astro-ph/9411077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9921
dc.subjectAstrophysics
dc.titleOpen clusters as tracers of the evolution of the Galaxy
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