Stellar population synthesis
| dc.creator | Ng, Y. K. | |
| dc.date | 1996-07-18 | |
| dc.date.accessioned | 2026-07-07T02:21:37Z | |
| dc.date.available | 2026-07-07T02:21:37Z | |
| dc.description | Monte-Carlo simulations of optical and near-infrared colour-magnitude diagrams in Baade's Window (l=1.0,b=-3.9) are compared with each other. The morphological structure of the red horizontal branch in those CMDs is likely due to a combination of extinction and age-metallicity of the stars from the bulge/bar. In contrast with the optical (V,I) passbands, the simulations indicate that it is feasible to separate metallicity from extinction with near-infrared data. | |
| dc.description | 4 pages LaTeX with 3 postscript figures included, uses psfig.tex and crckapb.sty, to appear in Proceedings of the 3rd DeNIS Euroconference "The impact of large scale near infrared surveys", P. Garzon-Lopez (ed.) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9607091 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9607091 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10570 | |
| dc.subject | Astrophysics | |
| dc.title | Stellar population synthesis | |
| dc.type | text |