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Stellar Mass Black Holes and Ultraluminous X-Ray Sources

We review the likely population, observational properties, and broad implications of stellar-mass black holes and ultraluminous x-ray sources. We focus on the clear empirical rules connecting accretion and outflow that have been established for stellar-mass black holes in binary systems in the past decade and a half. These patterns of behavior are probably the keys that will allow us to understand black hole feedback on the largest scales over cosmological time scales.

preprint2012arXivOpen access
Rob FenderTomaso Belloni
astro-ph.HE
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Open access2 authors1 topic
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Rob FenderTomaso Belloni

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