Models of ultraluminous X-ray sources with intermediate-mass black holes

Models of ultraluminous X-ray sources with intermediate-mass black holes

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We have computed models for ultraluminous X-ray sources ( ULXs) consisting of a black hole accretor of intermediate mass (IMBH; e.g., ~1000 M⊙) and a captured donor star. For each of four different sets of initial donor masses and orbital separations we computed 30,000 binaryevolution models using a...

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Bibliographic Details
Main Authors:	Madhusudhan, N, Justham, S, Nelson, L, Paxton, B, Pfahl, E, Podsiadlowski, P, Rappaport, S
Format:	Journal article
Published:	American Astronomical Society 2006
Subjects:	black hole physics galaxies: star clusters accretion, accretion disks X-rays: binaries

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