Observational evidence for stellar-mass black holes

  • Jorge Casares
  • Published 2005

Abstract

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… (More)

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Cite this paper

@inproceedings{Casares2005ObservationalEF, title={Observational evidence for stellar-mass black holes}, author={Jorge Casares}, year={2005} }