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Stellar population synthesis | | Y.K. Ng
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18 Jul 1996 | | Subject: | astro-ph | | Affiliation: | IAP, Paris, France | | Abstract: | 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. | | Source: | arXiv, astro-ph/9607091 | | Services: | Forum | Review | PDF | Favorites | |
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