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On the dynamic formation of accreting intermediate-mass black holes

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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.

Keywords: Accreting sources; Intermediate-mass black holes; Ultraluminous X-ray sources

Document Type: Research Article

DOI: http://dx.doi.org/10.1080/10556790701300751

Affiliations: 1: Sternberg Astronomical Institute, Moscow, Russia 2: Department of Physics, Moscow State University, Moscow, Russia 3: Sternberg Astronomical Institute, Moscow, Russia,Department of Physics, Moscow State University, Moscow, Russia 4: Department of Physics and Astronomy, Northwestern University, Illinois, USA 5: Joint Institute for Laboratory Astrophysics (Space) and Department of Astrophysical and Planetary Sciences, University of Colorado, Colorado, USA

Publication date: February 1, 2007

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