Models of ultraluminous X-ray sources with intermediate-mass black holes
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...
| Main Authors: | , , , , , , |
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| Format: | Journal article |
| Published: |
American Astronomical Society
2006
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| Subjects: |