Dynamics of the flute instability in accretion disks of AGN

Details Dynamics of the flute instability in accretion disks of AGN Dynamics of the flute instability in accretion disks of AGN

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39...23m&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 1, pp.23-25

Physics

Scientific paper

A new model for the accretion flows onto black holes is suggested. The model provides the high-frequency radiation from AGNs. The possibility of plasma retention by the magnetic field is discussed. It is shown that due to development of the flute instability the region where the magnetic and kinetic pressures are equal to each other can be located farther from the central object than the last stable Kepplerian orbit.

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