A local stability analysis of an isothermal disc with three- dimensional magnetic fields

Details A local stability analysis of an isothermal disc with three- dimensional magnetic fields A local stability analysis of an isothermal disc with three- dimensional magnetic fields

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.288..965y&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 288, Issue 4, pp. 965-972.

Astronomy and Astrophysics

Astronomy

3

Accretion, Accretion Discs, Instabilities, Magnetic Fields.

Scientific paper

The instability of an isothermal magnetized accretion disc is examined. It is shown that the radial and the azimuthal magnetic fields B_r, B_phi are dominant in enhancing the instability of the magneto-acoustic modes, and that the radial pulsational oscillations are larger than those in the z direction. Finally, we use our model to explain the variability of FU Orionis and T Tauri stars.

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