Colour-Magnitude Diagrams from microlensing projects and galactic structure
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/9607089,
title = {Colour-Magnitude Diagrams from microlensing projects and galactic structure},
author = {Y. K. Ng},
journal= {arXiv preprint arXiv:astro-ph/9607089},
year = {2007}
}
Comments
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.)