Observational evidence for stellar-mass black holes

@inproceedings{Matt2005ObservationalEF,
  title={Observational evidence for stellar-mass black holes},
  author={Giorgio Matt},
  year={2005}
}
Radial velocity studies of X-ray binaries provide the most solid evidence for the existence of stellar-mass black holes. We currently have 20 confirmed cases, with dynamical masses in excess of 3 M⊙. Accurate masses have been obtained for a subset of systems which gives us a hint at the mass spectrum of the black hole population. This review summarizes the history of black hole discoveries and presents the latest results in the field. 
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