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.date1995-04-20
dc.date1995-07-05
dc.date.accessioned2026-07-07T08:58:17Z
dc.date.available2026-07-07T08:58:17Z
dc.descriptionX-ray binary population at the Galactic center is proposed here to form as a result of a starburst, which is synthesized by using the ``Scenario Machine'' code of binary star evolution. 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.
dc.description4 pages, 1 figure, uuencoded compressed postscript
dc.identifierhttps://arxiv.org/abs/astro-ph/9504066
dc.identifierhttp://arxiv.org/abs/astro-ph/9504066
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147265
dc.subjectAstrophysics
dc.titlePopulation synthesis of X-ray sources at the Galactic center
dc.typetext

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