Pulsational instability of relativistic accretion disks and its connection to the periodic X-ray time variability of NGC 6814

Details Pulsational instability of relativistic accretion disks and its connection to the periodic X-ray time variability of NGC 6814 Pulsational instability of relativistic accretion disks and its connection to the periodic X-ray time variability of NGC 6814

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44..529h&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 5, p. 529-535.

Astronomy and Astrophysics

Astronomy

22

Accretion Disks, Active Galactic Nuclei, Magnetohydrodynamic Stability, Plasma Oscillations, Relativistic Plasmas, X Ray Sources, Black Holes (Astronomy), Periodic Variations

Scientific paper

It has been noted that the innermost region of accretion disks around relativistic compact objects is unsteady under certain conditions. This paper presents new results of numerical simulations to demonstrate the overall behavior of unstable disks. The possible connection of this type of disk oscillations with the periodic X-ray time variability of NGC 6814 is discussed.

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