The stability of an isothermal, magnetized and causally limited viscosity accretion disk

Details The stability of an isothermal, magnetized and causally limited viscosity accretion disk The stability of an isothermal, magnetized and causally limited viscosity accretion disk

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.232..293y&link_type=abstract

Astrophysics and Space Science, Volume 232, Issue 2, pp.293-306

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The stability of an isothermal, magnetized and causally limited viscosity accretion disk is examined in this paper. We find that the viscous modes are always stable throughout the disk, and the magneto-acoustic modes are pulsationally unstable. The results show that the Mach numbers do effect the instabilities of the disk and the magnetic field enhances the instability property of the radial oscillation. Our results are useful for understanding the time variations of AGN.

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