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Population synthesis of X-ray sources at the Galactic center

S. B. Popov·V. M. Lipunov·L. M. Ozernoy·K. A. Postnov·M. E. Prokhorov
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Abstract

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.

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S. B. Popov, V. M. Lipunov, L. M. Ozernoy, K. A. Postnov, M. E. Prokhorov. 1995-10-01. Population synthesis of X-ray sources at the Galactic center. https://arxiv.org/abs/astro-ph/9509155

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