From Young to Old: Spectral Models for Star Cluster Systems
| dc.creator | Alvensleben, Uta Fritze -- v. | |
| dc.creator | Anders, Peter | |
| dc.creator | de Grijs, Richard | |
| dc.date | 2003-10-21 | |
| dc.date.accessioned | 2026-07-07T02:10:43Z | |
| dc.date.available | 2026-07-07T02:10:43Z | |
| dc.description | Evolutionary synthesis models for star clusters of various metallicities including gaseous emission during the lifetime of the ionising stars are used to model star cluster systems comprising two populations: an old metal-poor globular clusters (GC) population similar to that of the Milky Way halo and a second GC population of arbitrary metallicity. We investigate the time evolution of color distributions and luminosity functions for the two GC populations in comparison with observations on E/S0 galaxies. We show that multi-passband data for GC populations give clues to the relative ages and metallicities of blue and red subpopulations and help constrain formation scenarios for their parent galaxies. | |
| dc.description | 2 pages, IAU JD06 Sydney 2003, to appear in ASP Conf. Ser., eds T. Bridges, D. Forbes | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310597 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310597 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6827 | |
| dc.subject | Astrophysics | |
| dc.title | From Young to Old: Spectral Models for Star Cluster Systems | |
| dc.type | text |