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Two stellar-mass black holes in the globular cluster M22

Author

Listed:
  • Jay Strader

    (Michigan State University
    Harvard-Smithsonian Center for Astrophysics)

  • Laura Chomiuk

    (Michigan State University
    Harvard-Smithsonian Center for Astrophysics
    National Radio Astronomy Observatory, PO Box O)

  • Thomas J. Maccarone

    (School of Physics and Astronomy, University of Southampton, Highfield SO17 IBJ, UK)

  • James C. A. Miller-Jones

    (International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, Western Australia 6845, Australia)

  • Anil C. Seth

    (University of Utah, Salt Lake City, Utah 84112, USA)

Abstract

Two flat-spectrum radio sources in the Milky Way globular cluster M22 are thought to be accreting stellar-mass black holes; the identification of two black holes in one cluster shows that the ejection of black holes from clusters is not as efficient as predicted by most models.

Suggested Citation

  • Jay Strader & Laura Chomiuk & Thomas J. Maccarone & James C. A. Miller-Jones & Anil C. Seth, 2012. "Two stellar-mass black holes in the globular cluster M22," Nature, Nature, vol. 490(7418), pages 71-73, October.
  • Handle: RePEc:nat:nature:v:490:y:2012:i:7418:d:10.1038_nature11490
    DOI: 10.1038/nature11490
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