Old Open Clusters as Tracers of Galactic Evolution
| dc.creator | Bragaglia, A. | |
| dc.creator | Tosi, M. | |
| dc.creator | Marconi, G. | |
| dc.creator | Carretta, E. | |
| dc.date | 1999-12-07 | |
| dc.date.accessioned | 2026-07-07T02:34:49Z | |
| dc.date.available | 2026-07-07T02:34:49Z | |
| dc.description | Old open clusters are useful tools to study the Galactic disk properties, both present and past. Populous samples with properties determined both accurately and homogenously are necessary to draw reliable conclusions. We present here our recent work in the field and introduce and discuss results on metallicities. | |
| dc.description | 6 pages, 3 figures, to appear in "The chemical evolution of the Milky Way: Stars versus clusters", September 20-24, Vulcano | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9912130 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9912130 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15397 | |
| dc.subject | Astrophysics | |
| dc.title | Old Open Clusters as Tracers of Galactic Evolution | |
| dc.type | text |