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Strong disk winds traced throughout outbursts in black-hole X-ray binaries

Author

Listed:
  • B. E. Tetarenko

    (University of Alberta)

  • J.-P. Lasota

    (Institut d’Astrophysique de Paris, CNRS et Sorbonne Universités
    Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences)

  • C. O. Heinke

    (University of Alberta)

  • G. Dubus

    (Université Grenoble Alpes, CNRS, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG))

  • G. R. Sivakoff

    (University of Alberta)

Abstract

Analysis of the light curves of outbursts in black-hole X-ray binaries suggests that throughout the accretion process mass is lost from the accretion disks through strong, magnetically driven disk winds.

Suggested Citation

  • B. E. Tetarenko & J.-P. Lasota & C. O. Heinke & G. Dubus & G. R. Sivakoff, 2018. "Strong disk winds traced throughout outbursts in black-hole X-ray binaries," Nature, Nature, vol. 554(7690), pages 69-72, February.
    • Handle: RePEc:nat:nature:v:554:y:2018:i:7690:d:10.1038_nature25159
    DOI: 10.1038/nature25159
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