Galactic metallicity distribution from open clusters
| dc.creator | Chen, L. | |
| dc.creator | Hou, J. L. | |
| dc.creator | Wang, J. J. | |
| dc.date | 2003-10-15 | |
| dc.date.accessioned | 2026-07-07T02:10:25Z | |
| dc.date.available | 2026-07-07T02:10:25Z | |
| dc.description | We have compiled two new Galactic open cluster catalogues. The first one has 119 objects with age, distance and metallicity data, while the second one has 144 objects with both absolute proper motion and radial velocity data, of which 45 clusters also with metallicity data available. An iron radial gradient of about $-0.063\pm$0.008 \dexkpc is obtained from our sample. By dividing clusters into age groups, we show that iron gradient was steeper in the past. A disk age-metallicity relation could very probably exist based on the current sample. | |
| dc.description | 2 pages, conference proceeding IAU General Assembly 2003, Sydney, Symposium 217: Recycling Intergalactic and Interstellar Matter. eds. P.-A. Duc, J. Braine and E. Brinks | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310395 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310395 | |
| dc.identifier | Astron. J. 2003, 125, 1397 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6738 | |
| dc.subject | Astrophysics | |
| dc.title | Galactic metallicity distribution from open clusters | |
| dc.type | text |