Accretion-Ejection Instability in black-hole binaries

Details Accretion-Ejection Instability in black-hole binaries Accretion-Ejection Instability in black-hole binaries

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..587..131v&link_type=abstract

GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP Conference Proceedings, Volume 587, pp. 131-134 (2001).

Astronomy and Astrophysics

Astrophysics

Quasars, Magnetohydrodynamics And Plasmas

Scientific paper

The Accretion-Ejection Instability has been proposed to explain the ``ubiquitous'' low frequency QPO of microquasars. This instability which occurs in the inner region of moderately magnetized disks has the the unique property that it can send toward the corona the energy and angular momentum from the disk. I will present recent results on the physics of the instability, and comparison with observations. In particular I will describe how it generates Alfven waves propagating the energy and angular momentum to the corona. .

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