The magnetic nature of disk accretion onto black holes
Astrophysics, abstract
astro-ph/0605390
From: Jon M. Miller [view email] Date: Tue, 16 May 2006 14:36:09 GMT (27kb)
The magnetic nature of disk accretion onto black holes
Authors:
J. M. Miller (1),
J. Raymond (2),
A. C. Fabian (3),
D. Steeghs (2),
J. Homan (4),
C. S. Reynolds (5),
M. van der Klis (6),
Rudy Wijnands (6) ((1) University of Michigan, (2) Harvard-Smithsonian CfA, (3) University of Cambridge, (4) MIT, (5) University of Maryland, (6) University of Amsterdam)
Comments: 15 pages, 2 color figures, accepted for publication in Nature.
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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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