The Future of Galaxy Populations
| dc.creator | Wyse, Rosemary F. G. | |
| dc.date | 1995-11-18 | |
| dc.date.accessioned | 2026-07-07T02:20:26Z | |
| dc.date.available | 2026-07-07T02:20:26Z | |
| dc.description | What the future holds for the stellar populations of the Milky Way Galaxy may (optimistically) be predicted by study of their past histories, as written in the chemical abundance distributions, angular momentum distributions, velocity dispersion tensor, ages and spatial structure of their constituent older stars. | |
| dc.description | 12 pages of text (plain tex); 3 figures available from author on request. Proceedings June 1995 ASP Symposium on `Clusters, Lensing and the Future of the Universe', eds V. Trimble | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9511083 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9511083 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10212 | |
| dc.subject | Astrophysics | |
| dc.title | The Future of Galaxy Populations | |
| dc.type | text |