Statistical Photometry of Faint Stars and Synthesis of Populations

Physics

Scientific paper

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Scientific paper

The authors review various attempts to develop models of stellar populations in the galaxy. Recent advances in the field of faint star counts are reviewed too. It is shown that unambiguous results cannot be obtained unless heterogeneous data from solar neighbourhood observations are taken into account (including kinematics, photometry, spectral classification of bright stars, intermediate magnitude stars in large fields and faint magnitude stars in small fields). The authors present a preliminary version of their model of the galaxy.

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