Resolving Extragalactic Star Clusters with HST/ACS
| dc.creator | Larsen, S. S. | |
| dc.date | 2007-07-02 | |
| dc.date.accessioned | 2026-07-07T08:13:31Z | |
| dc.date.available | 2026-07-07T08:13:31Z | |
| dc.description | With HST, colour-magnitude diagrams (CMDs) can be obtained for young star clusters well beyond the Local Group. Such data can help constrain cluster ages and metallicities, and also provide a reference against which intermediate- and high mass stellar models can be compared. Here, CMDs are presented for two massive (>10^5 Msun) clusters and compared with Padua and Geneva isochrones. The problem of the ratio of blue to red supergiants is also addressed. | |
| dc.description | 4 pages, incl. 2 figures. To appear in the proceedings of the 41st ESLAB Symposium, "The impact of HST on European astronomy", ed. G. De Marchi & F. D. Macchetto (Berlin: Springer), in press | |
| dc.identifier | https://arxiv.org/abs/0707.0205 | |
| dc.identifier | http://arxiv.org/abs/0707.0205 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/132796 | |
| dc.subject | Astrophysics | |
| dc.title | Resolving Extragalactic Star Clusters with HST/ACS | |
| dc.type | text |