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Mass Measurements of Stellar and Intermediate-Mass Black Holes

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Abstract

We discuss the method, and potential systematic effects therein, used for measuring the mass of stellar-mass black holes in X-ray binaries. We restrict our discussion to the method that relies on the validity of Kepler’s laws; we refer to this method as the dynamical method. We briefly discuss the implications of the mass distribution of stellar-mass black holes and provide an outlook for future measurements. Further, we investigate the evidence for the existence of intermediate-mass black holes i.e. black holes with masses above 100 M⊙, the limit to the black hole mass that can be produced by stellar evolution in the current Universe.

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Acknowledgements

We thanks Cristina Zurita, Andrew Cantrell and Rob Hynes for providing us with Figs. 5, 6 and 11, respectively. J.C. acknowledges support by the Spanish Ministerio de Economía y Competitividad (MINECO) under grant AYA2010-18080.

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Authors and Affiliations

  1. Instituto de Astrofísica de Canarias, 38205, La Laguna, S/C de Tenerife, Spain

    J. Casares

  2. Departamento de Astrofísica, Universidad de La Laguna, 38206, La Laguna, S/C de Tenerife, Spain

    J. Casares

  3. SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands

    P. G. Jonker

  4. Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL, Nijmegen, The Netherlands

    P. G. Jonker

  5. Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA, 02138, USA

    P. G. Jonker

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Casares, J., Jonker, P.G. Mass Measurements of Stellar and Intermediate-Mass Black Holes. Space Sci Rev 183, 223–252 (2014). https://doi.org/10.1007/s11214-013-0030-6

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