  We model the evolution of the selected types of X-ray sources (both with BHs
and NSs) for the star formation burst at the Galactic center. For the currently
assumed starburst age of 4-7 millions years, our results are consistent with
the recent {\it GRANAT} X-ray observations of the Galactic center and predict a
substantial number of X-ray binaries with black holes. In addition we made a
very simple model of the spatial distribution of the X-ray sources, which is
also consistent with the {\it GRANAT} observations. The results can be applied
to other starformation regions.
