

Author: Kuranov A. G.
Publisher: Taylor & Francis Ltd
ISSN: 1055-6796
Source: Astronomical and Astrophysical Transactions, Vol.26, Iss.1-3, 2007-02, pp. : 87-89
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Abstract
We compute the probability that intermediate-mass black holes (IMBHs) capture companions owing to dynamic interactions and appear as accreting sources and we explore the possibility that the accreting IMBHs would appear as ultraluminous X-ray sources.
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