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The magnetic nature of disk accretion onto black holes

J. M. Miller·J. Raymond·A. C. Fabian·D. Steeghs·J. Homan·C. S. Reynolds·M. van der Klis·Rudy Wijnands
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Abstract

Although disk accretion onto compact objects - white dwarfs, neutron stars, and black holes - is central to much of high energy astrophysics, the mechanisms which enable this process have remained observationally elusive. Accretion disks must transfer angular momentum for matter to travel radially inward onto the compact object. Internal viscosity from magnetic processes and disk winds can in principle both transfer angular momentum, but hitherto we lacked evidence that either occurs. Here we report that an X-ray-absorbing wind discovered in an observation of the stellar-mass black hole binary GRO J1655-40 must be powered by a magnetic process that can also drive accretion through the disk. Detailed spectral analysis and modeling of the wind shows that it can only be powered by pressure generated by magnetic viscosity internal to the disk or magnetocentrifugal forces. This result demonstrates that disk accretion onto black holes is a fundamentally magnetic process.

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J. M. Miller, J. Raymond, A. C. Fabian, D. Steeghs, J. Homan, C. S. Reynolds, M. van der Klis, Rudy Wijnands. 2006-05-16. The magnetic nature of disk accretion onto black holes. https://doi.org/10.1038/nature04912

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