Population synthesis of X-ray sources at the Galactic center

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dc.creatorPopov, S. B.
dc.creatorLipunov, V. M.
dc.creatorOzernoy, L. M.
dc.creatorPostnov, K. A.
dc.creatorProkhorov, M. E.
dc.date1995-10-01
dc.date.accessioned2026-07-07T02:20:14Z
dc.date.available2026-07-07T02:20:14Z
dc.descriptionWe 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.
dc.description8 pages, 3 figures, uuencoded gzip compressed postscript. will be presented as a poster at the conference "From Stars To Galaxies. The Impact of Stellar Physics on Galaxy Evolution"
dc.identifierhttps://arxiv.org/abs/astro-ph/9509155
dc.identifierhttp://arxiv.org/abs/astro-ph/9509155
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10148
dc.subjectAstrophysics
dc.titlePopulation synthesis of X-ray sources at the Galactic center
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