Colour-Magnitude Diagrams from microlensing projects and galactic structure
Abstract
Description
The results, obtained with the stellar population synthesis technique, are summarized for galactic structure and stellar population studies of our Galaxy. Emphasis is put on the analysis (extinction, disc structure, bar population) of the OGLE colour-magnitude diagram from Baade's Window.
5 pages, LaTeX, 7 postscript figures included, uses psfig.tex and conf_iap.sty, to appear in Proceedings of the 12th IAP Colloquium "Variable stars and the astrophysical returns of microlensing surveys", R. Ferlet and J.-P. Maillard (eds.)
5 pages, LaTeX, 7 postscript figures included, uses psfig.tex and conf_iap.sty, to appear in Proceedings of the 12th IAP Colloquium "Variable stars and the astrophysical returns of microlensing surveys", R. Ferlet and J.-P. Maillard (eds.)